2.1 Review of the literature

For the purposes of the review below, early time is qualitatively defined as the transient time period during which the relaxation of the initial configuration of the solute is important to the dynamics of the Taylor dispersion process. It is possible to broadly characterize the different mathematical approaches for describing Taylor dispersion in the transient, early-time regime as outlined below.

(i) Kramers–Moyal-like expansions. By far the most popular approach has been the proposition that the macroscale solution can be expressed as an infinite series of spatial derivatives of the average concentration. Several variations of this approach have been attempted, and they are represented in the works of Gill et al. (Gill & Sankarasubramanian Reference Gill and Sankarasubramanian1970, Reference Gill and Sankarasubramanian1971), Chatwin (O’Hara Reference O’Hara1969; Chatwin Reference Chatwin1970, Reference Chatwin1972), Degance & Johns (Reference Degance and Johns1978a,Reference Degance and Johnsb) and Mauri (Reference Mauri1991). Balakotaiah, Chang & Smith (Reference Balakotaiah, Chang and Smith1995) used centre manifold theory to develop a macroscale formulation that is identical to that of Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970). The resolution of the centre manifold model was improved by Watt & Roberts (Reference Watt and Roberts1996) by constructing a multi-mode model for dispersion in channels. These authors considered a two-component model that follows the same trend of thought of the zonal models by Chikwendu & Ojiakor (Reference Chikwendu and Ojiakor1985), Chikwendu (Reference Chikwendu1986a,Reference Chikwendub). The work by Yu (Reference Yu1976, Reference Yu1979) is interesting in that it began as a formal eigenfunction expansion for an unsimplified version of the convection–diffusion equation by assuming that expansions in Bessel functions were possible. After a formal integral solution was developed, the term arising from the initial conditions was discarded, and the remaining integrations of the Bessel functions were expanded in a power series. The result was a solution in an infinite series of derivatives of all orders, much like the Kramers–Moyal-type expansions discussed above. Although originally promoted as being more capable than the models of Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970), a sequence of comments (Gill & Subramanian Reference Gill and Subramanian1980; Yu Reference Yu1980) established that the two methods are, at least to order 3, identical. The works by Westerterp, Dil’man & Kronberg (Reference Westerterp, Dil’man and Kronberg1995) and Kronberg, Benneker & Westerterp (Reference Kronberg, Benneker and Westerterp1996) are of this type, but in that work the iterative process was truncated at order 2. One unique feature of those works is that mixed derivative terms were maintained, and this ultimately led to a macroscale form that had hyperbolic (rather than parabolic) features. We note that the work by Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970) also derived hyperbolic terms in their approach, but ultimately eliminated those terms on the basis of their assumed macroscale form. More recently, Wu & Chen (Reference Wu and Chen2014) used an expansion involving spatial derivatives up to ninth order. Although their results compared well with previously reported numerical results, they did not recognize that their solutions included significant negative concentrations outside of a limited domain. This kind of error was corrected in a later paper (Wang & Chen Reference Wang and Chen2016). Other works (Mercer & Roberts Reference Mercer and Roberts1990, Reference Mercer and Roberts1994; Balakotaiah et al. Reference Balakotaiah, Chang and Smith1995) also considered higher-order expansions and addressed the issue of negative concentrations.

(ii) Direct solutions. In the direct solutions, the focus has been to solve the convection–diffusion mass balance equation in the tube directly using an eigenfunction expansion. This is a challenging task, because the conventional methods (e.g. separation of variables) used to determine closed-form expressions for the Green’s function do not work with this problem, primarily because the convection term mixes both radial and longitudinal independent variables. The first direct solutions appear to be those of Philip (Reference Philip1963). For that work, however, the solution sought was initially of the form of a diffusion equation (similar to the more general approach of Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970)), which automatically excluded certain forms of the initial condition (with roughly the same reasoning discussed by Degance & Johns (Reference Degance and Johns1980)). The paper proposed a solution as a series of the confluent hypergeometric functions $_{1}F_{1}$. The papers by Tseng & Besant (Reference Tseng and Besant1970, Reference Tseng and Besant1972) assumed the same solution as did Philip (Reference Philip1963) (and were subject to the same restrictions), but managed to find simplifications that yielded solutions in terms of Bessel $\text{J}_{0}$ functions, the roots of the Bessel $\text{J}_{1}$ function and the error function. In the work by Stokes & Barton (Reference Stokes and Barton1990), a Fourier transformation method was used, but the results had to be inverted numerically; as such, it is difficult to compare these results with other efforts.

(iii) Asymptotic (perturbation) solutions. A number of perturbation-type solutions have been proposed, and it is not possible to cleanly categorize solutions from other approaches as being free from perturbation-like arguments. However, more classical perturbation-type expansions have been investigated by Vrentas & Vrentas (Reference Vrentas and Vrentas1988, Reference Vrentas and Vrentas2000). The paper by Lighthill (Reference Lighthill1966) is of this form, as was the extension proposed by Chatwin (Reference Chatwin1976, Reference Chatwin1977); both of these solutions required the time to be small compared to a characteristic diffusive time scale. Fife & Nicholes (Reference Fife and Nicholes1975) conducted a conventional perturbation analysis, but, importantly, recognized the potential influence of initial source terms, which is somewhat unique. Phillips and Kaye examined the asymptotic (but direct) solutions for $Pe\rightarrow \infty$ for both large $z$ (Reference Phillips and Kaye1996), and short times (Reference Phillips and Kaye1997); both solutions neglected longitudinal diffusion. Such solutions have generally been very successful when used in their range of validity (which generally involves either long or short times, and/or large or small Péclet numbers).

(iv) Moment methods. The early paper by Aris (Reference Aris1956) presented the first moment-based method for Taylor dispersion. Although the paper purported to eliminate the constraints proposed by Taylor (Reference Taylor1954), in fact the method is technically only suitable for asymptotic estimates of the dispersion coefficient, although some transient results were presented for particular initial conditions. Moment methods focus on determining the spatial moments of the concentration field rather than its mean value (which, quite usefully, simplifies the analysis), often with the tacit assumption that the effective parameters of the averaged mass balance equation can be determined directly from the moments. Again, it is difficult to categorize approaches as uniquely moment based, since many approaches compute moments regardless of the underpinning mathematical methods used. A number of researchers have extended moment method into the preasymptotic regime, including the works of Horn (Reference Horn1971), Chatwin (Reference Chatwin1977), Degance & Johns (Reference Degance and Johns1978b), Latini & Bernoff (Reference Latini and Bernoff2001) and Dentz & Carrera (Reference Dentz and Carrera2007). The moment technique has become particularly popular in describing Taylor-like flows in stratified media (e.g. Fried & Combarnous Reference Fried and Combarnous1971; Lake & Hirasaki Reference Lake and Hirasaki1981; Valocchi Reference Valocchi1989), downstream contaminant release in rivers (Smith Reference Smith1984), among many others. The method inherently assumes that a finite number of moments suitably defines the transport behaviour of the system, an assumption that is technically only true for specific initial conditions or in the near-asymptotic regime (this issue is discussed further in § 2.2).

(v) Non-local formulations. Few non-local formulations (containing terms with either time or space integrations in the transport equation) have been proposed for this problem. Although not specific to the Taylor problem, the work of Deng & Cushman (Reference Deng and Cushman1995) is of this type, and somewhat set the standard for non-local equations of the convection–dispersion type (however, in a more general context, the work of Eringen (Reference Eringen1978) was ground-breaking for non-local balance equations). The paper by Wood & Valdés-Parada (Reference Wood and Valdés-Parada2013) also proposed non-local formulations from the volume averaging perspective, although they were also not specific to the Taylor dispersion problem. In the report of Smith (Reference Smith1981a), one of the first non-local formulations to the Taylor problem was outlined. The developments of that paper were also guided by a Kramers–Moyal-type expansion, and thus lead to hyperbolic expressions with mixed derivatives as well as more general convolution-integral expressions (depending on the order of the truncation, and where in the analysis the truncations are performed). The work by Jones & Young (Reference Jones and Young1994) also used a variation of this approach, but in an asymptotic framework (also capitalizing on the centre manifold theory). In this theory, the results were able to capture some features of the early-time behaviour, but were not able to capture exponentially decaying-in-time modes; most likely, this was because the initial condition was not represented as a source term in the averaged equation.

(vi) Formulations that include an initial condition source. Most studies on Taylor dispersion have not been overly interested in the relaxation of the initial condition; often, the only initial conditions examined are either uniform pulses, or delta-like impulses (Vedel, Hovad & Bruus Reference Vedel, Hovad and Bruus2014). Few papers have been developed with the realization that the initial condition can manifest as a decaying source term in the averaged mass balance when more complex initial conditions are considered. Philip (Reference Philip1963) was aware that essentially forcing the upscaled mass balance to be of a convection–dispersion form would limit the choices available for the initial condition. The importance of the initial condition was also apparent to Lighthill (Reference Lighthill1966), although he was not able to complete a general analysis for his solution. In a series of papers, Gill and Sankarasubramanian derived macroscale models for unsteady solute dispersion considering uniform (Gill & Sankarasubramanian Reference Gill and Sankarasubramanian1970) and non-uniform (Gill & Sankarasubramanian Reference Gill and Sankarasubramanian1971; Sankarasubramanian & Gill Reference Sankarasubramanian and Gill1973) slugs as initial conditions. Connections between these works and the developments presented here are derived in additional detail in the supplementary material. The work by Yu (Reference Yu1979) began by including the initial condition in the macroscale balance, but later this term was dropped resulting in a final theory that does not have a source arising from the initial configuration of the system. In the papers by Degance and Johns (Reference Degance and Johns1978b, Reference Degance and Johns1980), the influence of the initial condition appeared as part of the theory. However, this work specifically considered a subset of possible initial conditions that work with the theory; in particular, separable product forms for the initial condition function were allowable, but sums of any two such functions were excluded (Degance & Johns Reference Degance and Johns1978a, § 4). Smith (Reference Smith1981b) identified and described three stages of unsteady dispersion from a point source using a ray-tracing method. Haber & Mauri (Reference Haber and Mauri1988) used a stochastic Markovian particle approach to examine the role of the initial condition; explicit asymptotic solutions were derived that illustrated that the observed dispersion coefficient depended upon the initial location of the particles. From a moment-based approach, the paper by Dentz & Carrera (Reference Dentz and Carrera2007) similarly considered delta-type impulses placed near the centre versus the wall initially; in that work, a distinction between local and global dispersion was defined to distinguish between the dispersion of a single delta impulse versus the dispersion observed for an extended source. Meng & Yang (Reference Meng and Yang2018) adopted a perspective similar to that of Dentz & Carrera (Reference Dentz and Carrera2007), but solved for the effective dispersion coefficient via eigenfunction expansions. They also found that the dispersion coefficient was a function of the initial configuration. In a sequence of two papers, Wood (Reference Wood2009, equations (17) and (29)) and Wood & Valdés-Parada (Reference Wood and Valdés-Parada2013) developed theories that explicitly included the influence of the initial condition as a source term in the averaged mass balance equation; this process was then used by Ostvar & Wood (Reference Ostvar and Wood2016) to describe the average diffusion and reaction from an initial (unmixed) configuration. Independently, Balakotaiah & Ratnakar (Reference Balakotaiah and Ratnakar2010) also developed balance expressions specifically for the Taylor dispersion problem in which source terms arising from the initial conditions were employed; a Kramers–Moyal-like expansion was used, but truncated at second order. This model had the ability to predict significant skewness in the distribution (Ratnakar & Balakotaiah Reference Ratnakar and Balakotaiah2011). While not unique to the models discussed, the prediction of skewness is an important check on the physics of the solution, since skewness should become non-zero at early times (even if the initial condition is symmetric), and it should asymptotically approach zero in the long-time regime.

In the remainder of the background section, we elaborate a little more on two specific issues that arise in the previous work summarized above: (i) The use of infinite-order (Kramers–Moyal-type) expansions, and (ii) the neglect of source terms arising from the initial condition.

2.2 Comments regarding Kramers–Moyal-type expansions

There are two significant problems with the infinite Kramers–Moyal-type expansions. First, because of the specific macroscale representation that is chosen, the resulting theory generates dispersion coefficients that may depend upon the initial condition (Degance & Johns Reference Degance and Johns1980). Second, research on the positivity of such series was apparently not known to progenitors of this approach. It is now known that such series either (i) converge exactly at second order and are strictly positive, or (ii) require all terms in order to converge and remain strictly positive (Marcinkiewicz Reference Marcinkiewicz1939; Pawula Reference Pawula1967). Although Kramers–Moyal expansions do (under appropriate conditions) converge, they do not converge in a highly physical way when strictly positive results are sought (as in the case of concentration). In other words, any finite truncation of a Kramers–Moyal expansion of order greater than two generates results that are negative in some parts of the domain. This problem has been discussed in the literature (e.g. Risken & Vollmer Reference Risken and Vollmer1979), but it is not generally well recognized in many disciplines outside of physics. The fact that negative concentrations are essentially guaranteed to occur for truncated expansions does not negate the usefulness of such expansions (Risken & Vollmer Reference Risken and Vollmer1979), but it does demand careful analysis and cautiousness when interpreting results. The problem of negative concentrations is most acute at early times (cf. Wood & Valdés-Parada (Reference Wood and Valdés-Parada2013, § 7)). Some of the problems associated with the Kramers–Moyal expansion can be eliminated by the recognition that such expansions can often be represented by non-local convolution expressions (Mercer & Roberts Reference Mercer and Roberts1990, Reference Mercer and Roberts1994). It is easy to show that a general non-local transport formulation can be written as an infinite-order expansion of local derivatives (this is illustrated in the supplementary material), although the converse of this is not always true. However, given that the macroscale equation form adopted in most of these examples is posited as an ansatz (e.g. Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970, equations (5) and (8))), then it might be reasonable to start directly with the convolution rather than the series form. For the specific problem of Taylor dispersion investigated in this paper, we are able to show that the solution is generally of a convolution form, giving further support that this kind of approach might have a stronger physical basis. Regardless, the non-local formulations generally avoid the problems associated with negative concentrations, and, in appropriate limits, reduce to more familiar local macroscale equations.

2.3 Influence of the initial conditions

As the review of the literature above suggests, the importance of the initial configuration at early times has been identified (although not resolved) previously. The problem can be most easily thought about in the context of layered media which, although not a tube, is still frequently represented as a Taylor dispersion process, (e.g. Fried & Combarnous Reference Fried and Combarnous1971; Gelhar, Gutjahr & Naff Reference Gelhar, Gutjahr and Naff1979; Lake & Hirasaki Reference Lake and Hirasaki1981; Chikwendu & Ojiakor Reference Chikwendu and Ojiakor1985; Chikwendu Reference Chikwendu1986a,Reference Chikwendub). Consider an initially uniform slug of solute in a system of horizontal layers of alternating high and low conductivity that is transported by a forward-flow/reverse-flow transport cycle. If a constant pressure gradient is applied for a short period of time such that the mean flow is right to left, the solute is displaced more in the high-velocity layers than in the low ones, leading to a spatially staggered final condition. Now, suppose the flow is stopped, and the pressure gradient reversed. The staggered configuration is the initial condition for a new transport process. Assuming that the total time interval is small enough so that transverse diffusion does not spread the solute very much between layers, the resulting motion is largely reversible. Upon reversing the flow field, a seemingly spread-out initial condition converges to become more organized (and less spread out). In the limit of zero diffusion, the final result of this first forward and then reversed transport would be exactly identical to the initial condition.

This kind of process creates some conceptual problems. Seemingly, the second moment of the process described above first increases and then, upon flow reversal, decreases in time. If one interprets the effective dispersion coefficient as being the classical one half of the time rate of change of the second spatial moment, then one predicts a negative dispersion coefficient for the second half of the cycle. This problem has been recognized in part as one that involves the distinction between spreading and mixing (e.g. Dentz & Carrera Reference Dentz and Carrera2007). However, one is still left with a macroscale equation that contains an apparent dispersion coefficient that can be negative under some conditions. The problem is of the inverse heat equation type, which is known to be ill posed (Weber Reference Weber1981). The solutions to such problems are lossy in general and can lead to significant problems in interpretation. Of more importance, however, is that such expressions are inconsistent with macroscale thermodynamics (Gray & Miller Reference Gray and Miller2009; Gray & Miller Reference Gray and Miller2014, chap. 10; Miller et al. Reference Miller, Valdés-Parada, Ostvar and Wood2018). Thus, if one hopes to solve problems in a manner consistent with the thermodynamics appropriate to the upscaled system, a negative dispersion coefficient is not a suitable choice. The use of higher-order diffusive-type equations (such as the method of Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970)) does not entirely remediate this problem. Although there are more degrees of freedom in these kinds of expansions to accommodate the influence of initial conditions, the fundamental problem is that the initial conditions enter the problem as source terms that are independent of the spatial derivatives of the average concentration. Thus, some initial configurations, when forced to fit a transport equation that contains no term representing a source, may predict non-physical behaviour for the dispersion coefficient, depending upon the underlying theory.

4.1 Preliminaries

In this paper, we upscale (or coarse grain) the system concentration field dynamics by simple spatial averaging against a weighting function. The underlying assumption in this approach is that the system can be sensibly represented by governing equations at more than one scale of resolution due to the multiscale (in space, time or both) characteristics of the system. Practically, this means that there exist averaging operators that sufficiently smooth spatial fluctuations in concentration such that an averaged behaviour is useful for understanding the system evolution. In this work, the averaging process is a somewhat modified form of volume averaging theory (which is frequently applied to porous materials, (Whitaker Reference Whitaker1999)), but we do not stress this point further.

In the remainder of this paper, we adopt cylindrical coordinates (figure 1); thus, for any function $\unicode[STIX]{x1D713}$, we have $\unicode[STIX]{x1D713}(\boldsymbol{r})=\unicode[STIX]{x1D713}(r,\unicode[STIX]{x1D703},z)$. The symbol $\boldsymbol{z}$ (set in bold font) is used exclusively to indicate the centroid of the averaging domain; therefore, this vector always has the component form $\boldsymbol{z}=(0,0,z)$. The averaging operator $\langle \cdot \rangle$ for Taylor dispersion is often defined with respect to weighting function $w$ by (Degance & Johns Reference Degance and Johns1978a)

(4.1)$$\begin{eqnarray}\langle \unicode[STIX]{x1D713}\rangle |_{(\boldsymbol{z},t)}=\int _{\boldsymbol{r}\in {\mathcal{V}}(\boldsymbol{z})}\unicode[STIX]{x1D713}(\boldsymbol{r},t)w(\boldsymbol{r}-\boldsymbol{z})\,\text{d}V(\boldsymbol{r}).\end{eqnarray}$$

Or, in the cylindrical coordinate system

(4.2)$$\begin{eqnarray}\langle \unicode[STIX]{x1D713}\rangle |_{(\boldsymbol{z},t)}=\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\int _{\unicode[STIX]{x1D703}=0}^{\unicode[STIX]{x1D703}=2\unicode[STIX]{x03C0}}\int _{r=0}^{r=a}\unicode[STIX]{x1D713}(r,\unicode[STIX]{x1D703},\unicode[STIX]{x1D701},t)w(r,\unicode[STIX]{x1D703},\unicode[STIX]{x1D701}-z)r\,\text{d}r\,\text{d}\unicode[STIX]{x1D703}\,\text{d}\unicode[STIX]{x1D701}.\end{eqnarray}$$

For this work, we adopt the classical area average, so that $w(\boldsymbol{r}-\boldsymbol{z})=w(r,\unicode[STIX]{x1D703},\unicode[STIX]{x1D701}-z)=1/(\unicode[STIX]{x03C0}a^{2})\unicode[STIX]{x1D6FF}(z-\unicode[STIX]{x1D701})$, which yields the conventional area average (note, other weighting functions have been adopted for Taylor dispersion, cf. Degance & Johns (Reference Degance and Johns1978a))

(4.3)$$\begin{eqnarray}\langle \unicode[STIX]{x1D713}\rangle |_{(\boldsymbol{z},t)}={\displaystyle \frac{1}{\unicode[STIX]{x03C0}a^{2}}}\int _{\unicode[STIX]{x1D703}=0}^{\unicode[STIX]{x1D703}=2\unicode[STIX]{x03C0}}\int _{r=0}^{r=a}\unicode[STIX]{x1D713}(r,\unicode[STIX]{x1D703},z,t)r\,\text{d}r\,\text{d}\unicode[STIX]{x1D703}.\end{eqnarray}$$

We refer to the filtered functions $\langle \unicode[STIX]{x1D713}\rangle$ as macroscale quantities to distinguish them from their microscale counterparts, $\unicode[STIX]{x1D713}$.

In addition to the definition of the averaging operator, it is also useful to define the following decompositions:

(4.4a)$$\begin{eqnarray}\displaystyle & c(\boldsymbol{r},t)=\langle c\rangle |_{(\boldsymbol{z},t)}+\tilde{c}(\boldsymbol{r},t) & \displaystyle\end{eqnarray}$$

(4.4b)$$\begin{eqnarray}\displaystyle & v_{z}(r)=U+\tilde{v}_{z}(r). & \displaystyle\end{eqnarray}$$

$U=\langle v_{z}\rangle |_{\boldsymbol{z}}$

$\tilde{c}$

$\tilde{v}_{z}$

(4.5a)$$\begin{eqnarray}\displaystyle & \langle \tilde{c}\rangle |_{(\boldsymbol{z},t)}=0, & \displaystyle\end{eqnarray}$$

(4.5b)$$\begin{eqnarray}\displaystyle & \langle \tilde{v}_{z}\rangle |_{\boldsymbol{z}}=0. & \displaystyle\end{eqnarray}$$

4.2 Averaging the microscale balance equation

To obtain the macroscale mass balance equation, we apply the averaging operator defined above to the microscale balance. Note that, although we have been careful to explicitly list the independent variables in the definitions above, we do so in the remainder of the paper only when it is necessary for emphasis or clarity. Upon applying the averaging operator (4.3) to the microscale mass balance equations, the upscaled problem takes the form

(4.6a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}={\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}-\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\right\rangle , & \displaystyle\end{eqnarray}$$

(4.6b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C. Macro 1a}\quad \langle c\rangle |_{(z,t)}=0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(4.6c)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C. Macro 1b}\quad -{\mathcal{D}}\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}=0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(4.6d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c\rangle |_{(z,0)}=\langle \unicode[STIX]{x1D711}\rangle |_{z}. & \displaystyle\end{eqnarray}$$

Several steps have been taken into account in order to derive (4.6a). First, interchange of the time derivative and the averaging operator is allowed within the accumulation term due to the fact that the averaging domain does not change with time. Thus we have

(4.7)$$\begin{eqnarray}\left\langle {\displaystyle \frac{\unicode[STIX]{x2202}c}{\unicode[STIX]{x2202}t}}\right\rangle ={\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}.\end{eqnarray}$$

Directing our attention to the diffusion term, the microscale boundary conditions lead to the identity

(4.8)$$\begin{eqnarray}\displaystyle \left\langle {\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}c}{\unicode[STIX]{x2202}z^{2}}}\right\rangle ={\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}. & & \displaystyle\end{eqnarray}$$

For the convection term, we have (on the basis of (4.4a)–(4.5b))

(4.9)$$\begin{eqnarray}\displaystyle \left\langle v_{z}{\displaystyle \frac{\unicode[STIX]{x2202}c}{\unicode[STIX]{x2202}z}}\right\rangle =U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}+\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\right\rangle . & & \displaystyle\end{eqnarray}$$

Finally, for the two macroscopic boundary conditions given in (4.6b) and (4.6c), we have imposed the condition that $\tilde{c}(r,\unicode[STIX]{x1D703},z)\rightarrow 0$ and $\unicode[STIX]{x2202}\tilde{c}/\unicode[STIX]{x2202}z(r,\unicode[STIX]{x1D703},z)\rightarrow 0$ as $|z|\rightarrow \infty$. Up to this point, we have employed no approximations to the result; the averaged model represented by (4.6a)–(4.6d) is exact, at least to the extent that the original microscale balance equations are valid.

5.1 Elimination of the non-local term

Rather than maintaining the non-local term, our approach is to develop reasonable constraints that allow us to neglect its influence. We do this by establishing characteristic time and length scales, and then developing constraints that indicate when the desired simplification is valid. Although these time and length scales can be given formal, computable definitions (e.g. such as defining them by the integral scale of the fields involved (Wood & Valdés-Parada Reference Wood and Valdés-Parada2013)), formal evaluation of scales is usually not necessary.

For the Taylor dispersion problem, there are several distinct length scales that can be defined. We have identified two important length scales in figure 2. The size of the macroscale length, $L_{0}$, is described as being approximately the size of the initial condition; however, the validity of this estimate depends upon the particular structure of the initial condition (this is discussed further in § 8.2). The characteristic length of the radial diffusion process is of the order of the tube radius, $a$, for this particular application.

Figure 2.

Length scales for the Taylor dispersion problem. The characteristic length associated with the initial solute configuration (illustrated in red) is $L_{0}$. Because of solute spreading, the generic length scale $L=L(t)$ (defined for all times) is asymptotically larger than $L_{0}$. This figure is meant to be primarily schematic; the actual initial conditions examined in this work are smoothed versions of similar configurations.

The non-local term and the convection term on the left-hand side of (5.3) are of the same order of magnitude. Thus, our desired restriction at this juncture would be to impose

(5.4)$$\begin{eqnarray}\tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}-\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\right\rangle \ll {\displaystyle \frac{{\mathcal{D}}}{r}}{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}r}}\left(r{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}r}}\right)+\cdots \,.\end{eqnarray}$$

For complex problems where one wishes to find all possible asymptotically simplified models, there are specific methods and algorithms that can be followed to construct the simplified models (see Yip (Reference Yip1996) for a fuller discussion). Because our restriction is rather simple (and because a full analysis is tedious), we only sketch out the result here. To start, we note that the left-hand side of (5.4) is always less than or equal to $\tilde{v}_{z}\unicode[STIX]{x2202}\tilde{c}/\unicode[STIX]{x2202}z$. Then, we non-dimensionalize and rearrange the problem as follows (where $Z=z/L_{0}$, $R=r/a$, $\tilde{V}_{z}=\tilde{v}_{z}/U$, $\tilde{C}=\tilde{c}/C_{0}$ and $C_{0}=\max (\tilde{\unicode[STIX]{x1D719}})$):

(5.5)$$\begin{eqnarray}\left({\displaystyle \frac{a^{2}U}{L_{0}{\mathcal{D}}}}\right)\tilde{V}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{C}}{\unicode[STIX]{x2202}Z}}={\displaystyle \frac{1}{R}}{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}R}}\left(R{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{C}}{\unicode[STIX]{x2202}R}}\right)+\cdots \,.\end{eqnarray}$$

Now, we set $\unicode[STIX]{x1D700}=a^{2}U/(L_{0}{\mathcal{D}})$. By assumption, $\tilde{V}_{z}\unicode[STIX]{x2202}\tilde{C}/\unicode[STIX]{x2202}Z=\boldsymbol{O}(1)$ and the first term on the right-hand side of (5.5) is of $\boldsymbol{O}(1)$. Examining

(5.6)$$\begin{eqnarray}\unicode[STIX]{x1D700}\tilde{V}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}Z}}={\displaystyle \frac{1}{R}}{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}R}}\left(R{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}R}}\right)+\cdots \,,\end{eqnarray}$$

it is clear that the left-hand side of this expression (and, hence, the left-hand side of (5.4)) can be neglected under the conditions

(5.7)$$\begin{eqnarray}{\displaystyle \frac{Ua}{{\mathcal{D}}}}{\displaystyle \frac{a}{L_{0}}}\ll 1\quad \text{or, equivalently, }Pe{\displaystyle \frac{a}{L_{0}}}\ll 1.\end{eqnarray}$$

The symbols ‘$\ll$’ and ‘$\boldsymbol{O}$’ have the conventional meanings adopted in perturbation theory (cf. Bender & Orszag (Reference Bender and Orszag1978, chapters 3.4 and 7)).

A few additional comments are helpful here. First, we note that this approximation may fail at early times if the concentration gradients in the initial condition are large (e.g. step functions); for these early-time solutions, the longitudinal derivative term would need to be maintained. In this work, we consider initial conditions that are reasonably smooth at $t=0$ (i.e. the first two derivatives are continuous, and correspond to a value of $L_{0}$ that is not much smaller than $a$). Second, this restriction is almost certainly overly severe once the relaxation of the initial condition has progressed for even a relatively small time. Often an approximation such as the inequality (5.4) is valid, even when the two sides are of the same order of magnitude. We describe the results of the error involved in this approximation in additional detail in § 8.2, where we compute it directly to show that the approximation is reasonable for the Péclet numbers investigated in this paper. It is worth noting that the constraint given in (5.7) is identical (except for a factor of 4) to the one imposed by Taylor (Reference Taylor1954)

(5.8)$$\begin{eqnarray}Pe_{T}={\displaystyle \frac{a^{2}}{4{\mathcal{D}}}}{\displaystyle \frac{U}{L}}\ll 1.\end{eqnarray}$$

Here, $Pe_{T}$ is the Taylor-type Péclet number, which arises naturally when we non-dimensionalize the transport equation. The diffusion time scale arises from considerations of the conventional free-field diffusion relationship with variance $\unicode[STIX]{x1D70E}^{2}=4{\mathcal{D}}t$ (and, hence, $L\sim \sqrt{4{\mathcal{D}}t}$). The convective time scale comes from a simple estimate of the $z-$derivative of the initial condition. With the exception of Taylor (Reference Taylor1954) and Aris (Reference Aris1956), the literature has tended to use the definition that is based on a simple ratio of the convective to diffusive fluxes, of the form (assuming both convective and diffusive fluxes are characterized by a length scale equal to the tube radius, $a$)

(5.9)$$\begin{eqnarray}Pe={\displaystyle \frac{Ua}{{\mathcal{D}}}}={\displaystyle \frac{4L}{a}}Pe_{T}.\end{eqnarray}$$

Note that for the simulations reported below with the parameters in table 1, $Pe_{T}=1$ corresponds to $Pe=80$.

Table 1.

Parameters used in the simulations.

With the approximation given by the inequality (5.4) and the use of Lagrangian coordinates, the resulting set of equations for $\tilde{c}$ becomes

(5.10a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}t}}={\displaystyle \frac{{\mathcal{D}}}{r}}{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}r}}\left(r{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}r}}\right)+{\displaystyle \frac{{\mathcal{D}}}{r^{2}}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\tilde{c}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D703}^{2}}}+{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\tilde{c}}{\unicode[STIX]{x2202}z^{2}}}-\underbrace{\tilde{v}_{z}(r)\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}}_{source}\quad (r,\unicode[STIX]{x1D703},z)\in {\mathcal{V}}, & \displaystyle\end{eqnarray}$$

(5.10b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C.1}\quad -{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}r}}=0\quad \text{at }r=0,a, & \displaystyle\end{eqnarray}$$

(5.10c)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C.2b}\quad \tilde{c}\rightarrow 0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(5.10d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C.2b}\quad -{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\rightarrow 0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(5.10e)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \tilde{c}(r,\unicode[STIX]{x1D703},z,0)=\underbrace{\tilde{\unicode[STIX]{x1D711}}(r,\unicode[STIX]{x1D703},z)}_{source}\quad (r,\unicode[STIX]{x1D703},z)\in {\mathcal{V}}. & \displaystyle\end{eqnarray}$$

The above simplified closure problem is a local, linear, non-homogeneous parabolic equation which has well-known solutions. With the conventional assumptions (e.g. boundedness of the initial condition, integrability of the initial condition, smoothness of the boundary conditions, etc.), the solution to the problem for solute transport can be put in an integral formulation as (cf. Polyanin & Nazaikinskii Reference Polyanin and Nazaikinskii2015)

(5.11)$$\begin{eqnarray}\displaystyle & & \displaystyle \tilde{c}(r,\unicode[STIX]{x1D703},z,t)\nonumber\\ \displaystyle & & \displaystyle \quad =\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}G(r,\unicode[STIX]{x1D70C},\unicode[STIX]{x1D703},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t)\tilde{\unicode[STIX]{x1D711}}(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},\unicode[STIX]{x1D701})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}\nonumber\\ \displaystyle & & \displaystyle \qquad -\int _{\unicode[STIX]{x1D70F}=0}^{\unicode[STIX]{x1D70F}=t}\!\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\!\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\!\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}G(r,\unicode[STIX]{x1D70C},\unicode[STIX]{x1D703},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})\tilde{v}_{z}(\unicode[STIX]{x1D70C})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(\unicode[STIX]{x1D701},\unicode[STIX]{x1D70F})}\,\text{d}\unicode[STIX]{x1D701}\text{d}\unicode[STIX]{x1D70F},\nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$

where $G(r,\unicode[STIX]{x1D70C},\unicode[STIX]{x1D703},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})$ is the Green’s function for this problem, which solves the initial and boundary-value problem given in appendix A by  (A 2a)–(A 2e).

6.1 Non-local solution

Using the unsimplified integral solution defined above by (5.11), we can develop a non-local but closed macroscale problem that takes the form

(6.1)$$\begin{eqnarray}{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}={\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}+{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}z}}\int _{\unicode[STIX]{x1D70F}=0}^{\unicode[STIX]{x1D70F}=t}\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\unicode[STIX]{x1D705}(z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(\unicode[STIX]{x1D701},\unicode[STIX]{x1D70F})}\,\text{d}\unicode[STIX]{x1D701}\,\text{d}\unicode[STIX]{x1D70F}-U\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}+s^{\ast }(z,t),\end{eqnarray}$$

where, for simplicity in notation, we have introduced

(6.2a)$$\begin{eqnarray}\unicode[STIX]{x1D705}(z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})=\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}\langle \tilde{v}_{z}G\rangle |_{(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})}\tilde{v}_{z}(\unicode[STIX]{x1D70C})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\end{eqnarray}$$

and

(6.2b)$$\begin{eqnarray}s^{\ast }(z,t)=-\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}\left.\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}G}{\unicode[STIX]{x2202}z}}\right\rangle \right|_{(\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t)}\tilde{\unicode[STIX]{x1D711}}(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},\unicode[STIX]{x1D701})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}.\end{eqnarray}$$

Non-local solutions have been proposed to describe a number of interesting transport phenomena (cf. Eringen Reference Eringen1978; Smith Reference Smith1981a; Cushman & Ginn Reference Cushman and Ginn1993; Deng, Cushman & Delleur Reference Deng, Cushman and Delleur1993; Neuman Reference Neuman1993; Deng & Cushman Reference Deng and Cushman1995). While they have some advantages, they also come with significant costs. Among these are that (i) analytical solutions are virtually non-existent, and (ii) because the solution at every point depends upon every other point in the domain, numerical schemes often have to deal with full rather than sparse matrices.

6.2 Localized solution

At this juncture in the analysis, we consider the effects of imposing two additional approximations: (i) the length scale constraint $a/L_{0}\ll 1$, and (ii) a time scale constraint $t^{\ast }/T^{\ast }\ll 1$ (where $t^{\ast }$ is a characteristic microscale process time, and $T^{\ast }$ is a characteristic macroscale process time). In appendix A we show that, for the Taylor problem in the range of Péclet numbers that we examine, the single constraint

(6.3)$$\begin{eqnarray}{\displaystyle \frac{a}{L_{0}}}\ll 1\end{eqnarray}$$

is sufficient to ensure that both the length and time scale constraints are met (a detailed derivation can be found in Wood & Valdés-Parada (Reference Wood and Valdés-Parada2013)). Note that this constraint is generally less restrictive (at least for $Pe>1$) than the constraint already imposed by the inequality (5.7). Technically, it is not necessary to impose any constraints on the problem. However, if we do not impose the inequalities (5.7) and (6.3), the result is a fully time- and space-non-local theory whose Green’s functions would be determined by an integro-differential equation with no known analytical solutions. Such a result would be unlikely to be simpler than directly solving the microscale balance given by (3.1a)–(3.1e).

With the constraints given by (5.7) and (6.3) in place, the localized solution for the set of balance equations associated with the solute ((5.10a)–(5.10e)) is given by (appendix A, (A 22))

(6.4)$$\begin{eqnarray}\tilde{c}(r,\unicode[STIX]{x1D703},z,t)=b(r,t)\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}+\unicode[STIX]{x1D6F7}(r,\unicode[STIX]{x1D703},z,t),\end{eqnarray}$$

where $b$ and $\unicode[STIX]{x1D6F7}$ are known as closure variables. These functions are defined in terms of the Green’s function by

(6.5a)$$\begin{eqnarray}\displaystyle & \displaystyle b(r,t;\tilde{v}_{z})=-\int _{\unicode[STIX]{x1D70F}=0}^{\unicode[STIX]{x1D70F}=t}\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}G(r,\unicode[STIX]{x1D70C},\unicode[STIX]{x1D703},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t-\unicode[STIX]{x1D70F})\tilde{v}_{z}(\unicode[STIX]{x1D70C})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}\,\text{d}\unicode[STIX]{x1D70F}, & \displaystyle \nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$

(6.5b)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6F7}(r,\unicode[STIX]{x1D703},z,t;\tilde{\unicode[STIX]{x1D711}})=\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}G(r,\unicode[STIX]{x1D70C},\unicode[STIX]{x1D703},\unicode[STIX]{x1D717},z,\unicode[STIX]{x1D701},t)\tilde{\unicode[STIX]{x1D711}}(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},\unicode[STIX]{x1D701})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}. & \displaystyle \nonumber\\ \displaystyle & & \displaystyle\end{eqnarray}$$

$b$

$\unicode[STIX]{x1D6F7}$

$\tilde{v}_{z}$

$\tilde{\unicode[STIX]{x1D711}}$

$\unicode[STIX]{x1D6F7}$

$\tilde{\unicode[STIX]{x1D711}}$

$\unicode[STIX]{x1D6F7}$

The solution form given by (6.4) is similar in form to the solution proposed by Paine, Carbonell & Whitaker (Reference Paine, Carbonell and Whitaker1983, equation (30)) for Taylor dispersion. Paine et al. (Reference Paine, Carbonell and Whitaker1983) correctly predicted that the solution for the deviation concentration should involve an independent function of time, they did not understand that this function is related to the initial condition for the problem (see appendix A). A fully local averaged balance equation can be developed, taking the form:

Local macroscale equation

(6.6a)$$\begin{eqnarray}\displaystyle & \displaystyle \underbrace{\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}\right|_{(z,t)}}_{accumulation}=\underbrace{D^{\ast }(t)\left.{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}\right|_{(z,t)}}_{diffusive\,transport}-\underbrace{U\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}}_{convective\,transport}+\underbrace{s^{\ast }(z,t)}_{\substack{ non\text{-}conventional \\ source}}, & \displaystyle\end{eqnarray}$$

(6.6b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C. Macro 1a}\quad \langle c\rangle |_{(z,t)}=0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(6.6c)$$\begin{eqnarray}\displaystyle & \displaystyle \text{B.C. Macro 1b}\quad -{\mathcal{D}}\left.{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}\right|_{(z,t)}=0\quad z\rightarrow \pm \infty , & \displaystyle\end{eqnarray}$$

(6.6d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c\rangle |_{(z,0)}=\langle \unicode[STIX]{x1D711}\rangle |_{z}\quad z\rightarrow \pm \infty . & \displaystyle\end{eqnarray}$$

(6.7a)$$\begin{eqnarray}\displaystyle & \displaystyle s^{\ast }(z,t)=-\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\unicode[STIX]{x1D6F7}}{\unicode[STIX]{x2202}z}}\right\rangle , & \displaystyle\end{eqnarray}$$

(6.7b)$$\begin{eqnarray}\displaystyle & \displaystyle D(t)=-\langle \tilde{v}_{z}b\rangle , & \displaystyle\end{eqnarray}$$

(6.7c)$$\begin{eqnarray}\displaystyle & \displaystyle D^{\ast }(t)={\mathcal{D}}+D(t). & \displaystyle\end{eqnarray}$$

$D$

$D^{\ast }$

$s^{\ast }$

$D^{\ast }$

$b$

$s^{\ast }$

$\unicode[STIX]{x1D6F7}$

The role of the source term is to account for the early-time memory of the initial distribution of the spatial deviations of the concentration. Although it is a source term in the balance equation, it is easy to show that the integral of this term over the domain $-\infty <z<\infty$ is identically zero (§ A.3). This indicates that the role of this term is only to redistribute mass within the domain; no mass is created or destroyed by this term.

Finally, a few comments regarding the effective parameters $s^{\ast }$ and $D^{\ast }$ are in order. First, we note that it can be shown that the effective dispersion coefficient, $D^{\ast }$ is a strictly positive function for all time, regardless of the initial conditions (§ A.5). As mentioned previously, this is a necessary condition for the problem if one wants the solution to be consistent with macroscopic scale thermodynamics (Miller et al. Reference Miller, Valdés-Parada, Ostvar and Wood2018). This has important repercussions for previous works that have suggested the use of negative dispersion coefficients; this is examined in detail in the Discussion section. Second, we note that the source term, $s^{\ast }$, like the function $\unicode[STIX]{x1D6F7}$, is an exponentially decreasing function of time (§ A.5). Therefore, $\unicode[STIX]{x1D6F7}$ decays toward zero as time grows large enough, recovering the conventional Taylor–Aris theory at asymptotic times. Although this term does decay to zero in time, the effect of this source term on the early stages of the diffusion–convection transport phenomenon is significant in some cases. This is discussed in additional detail in the following sections.

In the remainder of this paper, we adopt a strictly local representation; ultimately, we are able to show that this is an appropriate approximation for our system and range of parameters. Readers interested in examining how the non-local formulation can be solved numerically are directed to the details outlined by Deng et al. (Reference Deng, Cushman and Delleur1993).

7.1 Analytical solution for the $b$-field

In appendix A, the Green’s function for the general problem is identified, and integrated. The result is (§ A.3)

(7.1)$$\begin{eqnarray}b(r,t)={\displaystyle \frac{1}{4}}{\displaystyle \frac{Ua^{2}}{{\mathcal{D}}}}\left({\displaystyle \frac{r^{2}}{a^{2}}}-{\displaystyle \frac{r^{4}}{2a^{4}}}-{\displaystyle \frac{1}{3}}\right)+{\displaystyle \frac{2Ua^{2}}{{\mathcal{D}}}}\mathop{\sum }_{n=1}^{\infty }{\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})\text{J}_{0}\left(\unicode[STIX]{x1D706}_{n}{\displaystyle \frac{r}{a}}\right)}{\unicode[STIX]{x1D706}_{n}^{3}\text{J}_{0}^{2}(\unicode[STIX]{x1D706}_{n})}}\exp \left(-\unicode[STIX]{x1D706}_{n}^{2}{\displaystyle \frac{{\mathcal{D}}}{a^{2}}}t\right).\end{eqnarray}$$

Note that $b$ is not a function of $\unicode[STIX]{x1D703}$ or $z$. The eigenvalues $\unicode[STIX]{x1D706}_{n}$ can be computed by solving

(7.2)$$\begin{eqnarray}\text{J}_{1}(\unicode[STIX]{x1D706}_{n})=0,\quad n=1,2,3,\ldots .\end{eqnarray}$$

Equation (7.1) is equivalent to equation (16) in the work of Gill & Sankarasubramanian (Reference Gill and Sankarasubramanian1970). We note additionally here that in this derivation, it has been explicitly assumed that the initial time is represented by $t=0$.

The effective parameters, $D^{\ast }$ and $s^{\ast }$ associated with the upscaled equation are given by (6.7a) and (6.7c). Substituting the two solutions above for $b$ and $\unicode[STIX]{x1D6F7}$ as required into the general expressions for the effective parameters gives the following results (§ A.5):

(7.3)$$\begin{eqnarray}{\displaystyle \frac{D^{\ast }(t)}{{\mathcal{D}}}}=\left(1+{\displaystyle \frac{1}{48}}{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}\right)-4{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}\mathop{\sum }_{n=1}^{\infty }\left({\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\right)^{2}\exp \left(-\unicode[STIX]{x1D706}_{n}^{2}{\displaystyle \frac{{\mathcal{D}}}{a^{2}}}t\right),\end{eqnarray}$$

where we note that

(7.4)$$\begin{eqnarray}{\displaystyle \frac{1}{48}}{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}=4{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}\mathop{\sum }_{n=1}^{\infty }\left({\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\right)^{2}.\end{eqnarray}$$

We can also express this result in a form that is independent of $Pe$

(7.5)$$\begin{eqnarray}\left({\displaystyle \frac{D^{\ast }(t)}{{\mathcal{D}}}}-1\right)Pe^{-2}={\displaystyle \frac{1}{48}}-4\mathop{\sum }_{n=1}^{\infty }\left({\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\right)^{2}\exp (-\unicode[STIX]{x1D706}_{n}^{2}\unicode[STIX]{x1D70F}_{d}^{\ast }).\end{eqnarray}$$

Here, we have defined the dimensionless diffusion time variable

(7.6)$$\begin{eqnarray}\unicode[STIX]{x1D70F}_{d}^{\ast }={\displaystyle \frac{{\mathcal{D}}}{a^{2}}}t,\end{eqnarray}$$

where $a^{2}/{\mathcal{D}}$ is the diffusive time scale as defined in (B 32). The dispersion coefficient predicted from this expression is plotted in figure 3. Note that (7.5) is an evolving function of time, reaching more than 99 % of the expected asymptotic value of $1/48$ for $\unicode[STIX]{x1D70F}_{d}^{\ast }\gtrsim 0.3$.

Figure 3.

Evaluation of the dynamics of the dispersion coefficient using the analytical solution given in (7.5).

7.2 Analytical solution for the $\unicode[STIX]{x1D6F7}$-field

For the $\unicode[STIX]{x1D6F7}$ field, the final results depend on the particular initial condition that is investigated. However, we can provide the following general integral solution (the solutions for particular initial conditions are discussed in the sections following):

(7.7)$$\begin{eqnarray}\unicode[STIX]{x1D6F7}(r,\unicode[STIX]{x1D703},z,t)=B_{0,0}(z,t)+\mathop{\sum }_{n=0}^{\infty }\mathop{\sum }_{m=1}^{\infty }B_{n,m}(\unicode[STIX]{x1D703},z,t)\text{J}_{n}\left({\displaystyle \frac{\unicode[STIX]{x1D706}_{nm}r}{a}}\right)\exp \left(-{\displaystyle \frac{\unicode[STIX]{x1D706}_{nm}^{2}{\mathcal{D}}}{a^{2}}}t\right),\end{eqnarray}$$

where, for convenience, we introduced the functions $B_{0,0}(z,t)$ and $B_{n,m}(\unicode[STIX]{x1D703},z,t)$, which are defined by

(7.8a)$$\begin{eqnarray}B_{0,0}(z,t)={\displaystyle \frac{1}{\unicode[STIX]{x03C0}a^{2}}}\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }G_{2}(z,\unicode[STIX]{x1D701},t)\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}\tilde{\unicode[STIX]{x1D711}}(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},\unicode[STIX]{x1D701})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}\end{eqnarray}$$

(7.8b)$$\begin{eqnarray}\displaystyle B_{n,m}(\unicode[STIX]{x1D703},z,t) & = & \displaystyle {\displaystyle \frac{A_{n}\unicode[STIX]{x1D706}_{nm}^{2}}{\unicode[STIX]{x03C0}a^{2}(\unicode[STIX]{x1D706}_{nm}^{2}-n^{2})\text{J}_{n}^{2}(\unicode[STIX]{x1D706}_{nm})}}\int _{\unicode[STIX]{x1D701}=-\infty }^{\unicode[STIX]{x1D701}=\infty }G_{2}(z,\unicode[STIX]{x1D701},t)\int _{\unicode[STIX]{x1D717}=0}^{\unicode[STIX]{x1D717}=2\unicode[STIX]{x03C0}}\cos [n(\unicode[STIX]{x1D703}-\unicode[STIX]{x1D717})]\nonumber\\ \displaystyle & & \displaystyle \times \,\int _{\unicode[STIX]{x1D70C}=0}^{\unicode[STIX]{x1D70C}=a}\text{J}_{n}\left(\unicode[STIX]{x1D706}_{nm}{\displaystyle \frac{\unicode[STIX]{x1D70C}}{a}}\right)\tilde{\unicode[STIX]{x1D711}}(\unicode[STIX]{x1D70C},\unicode[STIX]{x1D717},\unicode[STIX]{x1D701})\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D70C}\,\text{d}\unicode[STIX]{x1D717}\,\text{d}\unicode[STIX]{x1D701}.\end{eqnarray}$$

Here, $G_{2}$ is the Green’s function in the axial direction and it is defined in appendix A (A 4b). The constants $A_{n}$ are given by $A_{1}=1$ and $A_{n}=2,n>1$. The eigenvalues $\unicode[STIX]{x1D706}_{nm}$ are the positive roots of the transcendental equation $\text{J}_{n}^{\prime }(\unicode[STIX]{x1D706}_{nm})=0$.

The results for the $s^{\ast }$ field depend upon the particular initial configuration that is specified; therefore, we cannot provide explicit expressions until the initial condition is identified. In general, the expression is given by (6.7a), which, using (7.7), can be put in the form

(7.9)$$\begin{eqnarray}s^{\ast }(z,t)=-\mathop{\sum }_{n=0}^{\infty }\mathop{\sum }_{m=1}^{\infty }{\displaystyle \frac{\unicode[STIX]{x2202}B_{n,m}}{\unicode[STIX]{x2202}z}}\left\langle \tilde{v}_{z}\text{J}_{n}\left({\displaystyle \frac{\unicode[STIX]{x1D706}_{nm}r}{a}}\right)\right\rangle \exp \left(-{\displaystyle \frac{\unicode[STIX]{x1D706}_{nm}^{2}{\mathcal{D}}}{a^{2}}}t\right).\end{eqnarray}$$

Because $s^{\ast }$ is a source term, the characteristics of the source can have a large impact on the solution. Explicit analytical expressions for a few specific initial conditions are derived in the next section. We note that for radially symmetric initial conditions, these general solutions are simplified somewhat due to symmetry (see § A.4).

As a final note, the functions $D^{\ast }$ and $s^{\ast }$ were developed explicitly for the case where the initial time is defined by $t=0$. If the initial time is some positive value, $T_{1}$, then the functions $D^{\ast }$ and $s^{\ast }$ should be specified as functions of the time since injection of the initial condition, $t^{\prime }$, where $t^{\prime }=t-T_{1}$. The important point is that $D^{\ast }$ and $s^{\ast }$ depend on time since injection of the initial condition, not on absolute time.

Figure 4.

Three-dimensional representations for the three types of the initial concentrations. The flow direction is left to right. Case B and C initial configurations have radial dependence. For visualization purposes, only a portion of the domain is shown.

7.3 Analytical solution for specific initial conditions

For this work, we consider three different initial conditions (illustrated in figure 4, where flow in the tube is from left to right), and provide the analytical solutions for $s^{\ast }$ for these three cases. Each initial condition is radially symmetric; this is not necessary for the general solution developed to this point, but to date we have found explicit series solutions only for these symmetry conditions (cf. the radially symmetric solution form for $\unicode[STIX]{x1D6F7}$ given in § A.4). Each case consists of initial conditions in which two concentration distributions are separated spatially (specifically, the centre of mass is separated by $L_{0}=20~\text{cm}$, see table 1). In order to avoid the singular points that arise when differentiating discontinuous initial distributions, these were weighted in the $z$-direction by a non-compact smoothing function. For each initial condition considered, the configuration could be decomposed into multiplicative radial and longitudinal components as follows:

(7.10)$$\begin{eqnarray}\unicode[STIX]{x1D711}(r,z)=c_{0}R_{1}(r)Z_{1}(z)+c_{0}R_{2}(r)Z_{2}(z).\end{eqnarray}$$

This multiplicative decomposition is not a necessary part of the solution, but it does aid in the subsequent determination of analytical solutions to the closure problem. In the longitudinal direction, the initial condition function was the same for each of the three cases, and was specified by

(7.11a)$$\begin{eqnarray}\displaystyle & \displaystyle Z_{1}(z)=\unicode[STIX]{x1D6FC}_{1}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6FD}_{1})^{2}}{\unicode[STIX]{x1D70E}_{1}^{2}}}\right), & \displaystyle\end{eqnarray}$$

(7.11b)$$\begin{eqnarray}\displaystyle & \displaystyle Z_{2}(z)=\unicode[STIX]{x1D6FC}_{2}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6FD}_{2})^{2}}{\unicode[STIX]{x1D70E}_{2}^{2}}}\right). & \displaystyle\end{eqnarray}$$

$\unicode[STIX]{x1D6FC}_{1}$

$\unicode[STIX]{x1D6FC}_{2}$

$\unicode[STIX]{x1D6FD}_{1}$

$\unicode[STIX]{x1D6FD}_{2}$

$\unicode[STIX]{x1D70E}_{1}$

$\unicode[STIX]{x1D70E}_{2}$

$R_{1}$

$R_{2}$

We note that a more accurate value for $L_{0}$ might be of the order of $\unicode[STIX]{x1D70E}_{1}$ and $\unicode[STIX]{x1D70E}_{2}$ rather than the spacing between the pulses. Note that with these estimates we have $a/\unicode[STIX]{x1D70E}_{1}=a/\unicode[STIX]{x1D70E}_{2}=1/3$. While this quantity is less than one, it is in a region of the constraint $a/L_{0}\ll 1$ that is somewhat unclear in terms of validity. However, we explicitly compute errors associated with these approximations in § 8.2; those results suggest that the approximation of separation of length scales is reasonably well met for the three problems investigated here.

7.3.1 Case A: radially uniform slugs

For this case, the initial condition is defined by two radially uniform slugs whose centre of mass is separated by $L_{0}$. The functions $R_{1}$ and $R_{2}$ are given by

(7.12a)$$\begin{eqnarray}\displaystyle & R_{1}(r)=1, & \displaystyle\end{eqnarray}$$

(7.12b)$$\begin{eqnarray}\displaystyle & R_{2}(r)=1 & \displaystyle\end{eqnarray}$$

i.e. there is no variation in the radial direction. For initial conditions with no radial variation, we have shown in appendix A that the solution for the source term is $s^{\ast }(z,t)=0$. This can also be seen through the closure problem for $\unicode[STIX]{x1D6F7}$ specified above. When initial conditions contain radially constant concentrations, the deviation concentrations are identically zero initially. This means that there are no source terms in the closure for $\unicode[STIX]{x1D6F7}$, and the problem generates only the zero solution.

7.3.2 Case B: linear radial distributions

For this case, each part of the initial condition was specified by a linear function. On the left (centred at $z=12.5~\text{cm}$) the concentration was maximum in the centre, and decreased linearly toward the wall. On the right (centred at $z=32.5~\text{cm}$) the concentration was greatest at the wall, and decreased linearly toward the centre. The functions $R_{1}$ and $R_{2}$ are given by

(7.13a)$$\begin{eqnarray}\displaystyle & \displaystyle R_{1}(r)=1-{\displaystyle \frac{r}{a}}, & \displaystyle\end{eqnarray}$$

(7.13b)$$\begin{eqnarray}\displaystyle & \displaystyle R_{2}(r)={\displaystyle \frac{r}{a}}. & \displaystyle\end{eqnarray}$$

For this case, the source term has been derived in appendix B. The result is

(7.14)$$\begin{eqnarray}\displaystyle s^{\ast }(z,t) & = & \displaystyle -4\unicode[STIX]{x03C0}c_{0}U\left[{\displaystyle \frac{\unicode[STIX]{x1D70E}_{1}\unicode[STIX]{x1D6FC}_{1}(z-\unicode[STIX]{x1D6EF}_{1}(t)-\unicode[STIX]{x1D6FD}_{1})}{\left(\unicode[STIX]{x1D70E}_{1}^{2}+4{\mathcal{D}}t\right)^{3/2}}}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6EF}_{1}(t)-\unicode[STIX]{x1D6FD}_{1})^{2}}{\unicode[STIX]{x1D70E}_{1}^{2}+4{\mathcal{D}}t}}\right)\right.\nonumber\\ \displaystyle & & \displaystyle -\left.{\displaystyle \frac{\unicode[STIX]{x1D70E}_{2}\unicode[STIX]{x1D6FC}_{2}(z-\unicode[STIX]{x1D6EF}_{2}(t)-\unicode[STIX]{x1D6FD}_{2})}{\left(\unicode[STIX]{x1D70E}_{2}^{2}+4{\mathcal{D}}t\right)^{3/2}}}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6EF}_{2}(t)-\unicode[STIX]{x1D6FD}_{2})^{2}}{\unicode[STIX]{x1D70E}_{2}^{2}+4{\mathcal{D}}t}}\right)\right]\nonumber\\ \displaystyle & & \displaystyle \times \,\mathop{\sum }_{n=1}^{\infty }{\displaystyle \frac{\boldsymbol{H}_{1}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{3}}}{\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\exp \left(-{\displaystyle \frac{\unicode[STIX]{x1D706}_{n}^{2}{\mathcal{D}}}{a^{2}}}t\right),\end{eqnarray}$$

where $\boldsymbol{H}_{1}$ is the Struve $H$ function (cf. equation (11.1.7) in Abramowitz & Stegun Reference Abramowitz and Stegun1965). The quantities $\unicode[STIX]{x1D6EF}_{1}$ and $\unicode[STIX]{x1D6EF}_{2}$ are the functions defining the motion of the centre of mass of the two portions (left and right) of the initial condition. They are specified by

(7.15a)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6EF}_{1}(t)=\left\{\begin{array}{@{}ll@{}}{\displaystyle \frac{7}{5}}Ut-{\displaystyle \frac{4}{15}}U{\displaystyle \frac{t^{3/2}}{\sqrt{t_{d}^{\ast }}}},\quad & \text{for }t<t_{d}^{\ast }\\ \unicode[STIX]{x1D6EF}_{1}(t_{d}^{\ast })+U(t-t_{d}^{\ast }),\quad & \text{for }t\geqslant t_{d}^{\ast }\end{array}\right. & \displaystyle\end{eqnarray}$$

(7.15b)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6EF}_{2}(t)=\left\{\begin{array}{@{}ll@{}}{\displaystyle \frac{4}{5}}Ut+{\displaystyle \frac{2}{15}}U{\displaystyle \frac{t^{3/2}}{\sqrt{t_{d}^{\ast }}}},\quad & \text{for }t<t_{d}^{\ast }\\ \unicode[STIX]{x1D6EF}_{2}(t_{d}^{\ast })+U(t-t_{d}^{\ast }),\quad & \text{for }t\geqslant t_{d}^{\ast },\end{array}\right. & \displaystyle\end{eqnarray}$$

where $t_{d}^{\ast }\equiv a^{2}/4{\mathcal{D}}$ is the diffusive time scale.

7.3.3 Case C: step radial distributions

For the third case, each part of the initial condition is specified by radial step functions that are complements of one another. The result is an initial condition that resembles a cylinder (with radius $a/2$) concentrated on the axis centred at $z=12.5~\text{cm}$, and a hollow cylinder (with radial thickness equal to $a/2$) centred at $z=32.5~\text{cm}$. The functions $R_{1}$ and $R_{2}$ are given by

(7.16a)$$\begin{eqnarray}\displaystyle & \displaystyle R_{1}(r)=\left\{\begin{array}{@{}ll@{}}1,\quad & 0\leqslant r\leqslant {\displaystyle \frac{a}{2}},\\ 0,\quad & {\displaystyle \frac{a}{2}}<r\leqslant a,\end{array}\right. & \displaystyle\end{eqnarray}$$

(7.16b)$$\begin{eqnarray}\displaystyle & \displaystyle R_{2}(r)=\left\{\begin{array}{@{}ll@{}}0,\quad & 0\leqslant r\leqslant {\displaystyle \frac{a}{2}},\\ 1,\quad & {\displaystyle \frac{a}{2}}<r\leqslant a.\end{array}\right. & \displaystyle\end{eqnarray}$$

These initial conditions were investigated separately by Degance & Johns (Reference Degance and Johns1978b). The solution for the source term is derived in appendix B, and the result is

(7.17)$$\begin{eqnarray}\displaystyle s^{\ast }(z,t) & = & \displaystyle 4c_{0}U\left[{\displaystyle \frac{\unicode[STIX]{x1D70E}_{1}\unicode[STIX]{x1D6FC}_{1}(z-\unicode[STIX]{x1D6EF}_{1}(t)-\unicode[STIX]{x1D6FD}_{1})}{(\unicode[STIX]{x1D70E}_{1}^{2}+4{\mathcal{D}}t)^{3/2}}}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6EF}_{1}(t)-\unicode[STIX]{x1D6FD}_{1})^{2}}{\unicode[STIX]{x1D70E}_{1}^{2}+4{\mathcal{D}}t}}\right)\right.\nonumber\\ \displaystyle & & \displaystyle -\left.{\displaystyle \frac{\unicode[STIX]{x1D70E}_{2}\unicode[STIX]{x1D6FC}_{2}(z-\unicode[STIX]{x1D6EF}_{2}(t)-\unicode[STIX]{x1D6FD}_{2})}{(\unicode[STIX]{x1D70E}_{2}^{2}+4{\mathcal{D}}t)^{3/2}}}\exp \left(-{\displaystyle \frac{(z-\unicode[STIX]{x1D6EF}_{2}(t)-\unicode[STIX]{x1D6FD}_{2})^{2}}{\unicode[STIX]{x1D70E}_{2}^{2}+4{\mathcal{D}}t}}\right)\right]\nonumber\\ \displaystyle & & \displaystyle \times \,\mathop{\sum }_{n=1}^{\infty }{\displaystyle \frac{\text{J}_{1}(\unicode[STIX]{x1D706}_{n}/2)\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}J_{0}^{2}(\unicode[STIX]{x1D706}_{n})}}\exp \left(-{\displaystyle \frac{\unicode[STIX]{x1D706}_{n}^{2}{\mathcal{D}}}{a^{2}}}t\right).\end{eqnarray}$$

Examples of this function are plotted in figure 5. Similar to the developments for the radially linear case, the centre of mass for the left and right components of the initial condition are given by

(7.18a)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6EF}_{1}(t)=\left\{\begin{array}{@{}ll@{}}{\displaystyle \frac{7}{4}}Ut-{\displaystyle \frac{1}{2}}U{\displaystyle \frac{t^{3/2}}{\sqrt{t_{d}^{\ast }}}},\quad & \text{for }t<t_{d}^{\ast },\\ \unicode[STIX]{x1D6EF}_{1}(t_{d}^{\ast })+U(t-t_{d}^{\ast }),\quad & \text{for }t\geqslant t_{d}^{\ast },\end{array}\right. & \displaystyle\end{eqnarray}$$

(7.18b)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D6EF}_{2}(t)=\left\{\begin{array}{@{}ll@{}}{\displaystyle \frac{3}{4}}Ut+{\displaystyle \frac{1}{6}}U{\displaystyle \frac{t^{3/2}}{\sqrt{t_{d}^{\ast }}}},\quad & \text{for }t<t_{d}^{\ast },\\ \unicode[STIX]{x1D6EF}_{2}(t_{d}^{\ast })+U(t-t_{d}^{\ast }),\quad & \text{for }t\geqslant t_{d}^{\ast }.\end{array}\right. & \displaystyle\end{eqnarray}$$

Following the material in appendix B as a guide, it should be relatively easy to develop analytical solutions for $s^{\ast }$ for other initial conditions of multiplicative form, assuming that the integration defined by (7.8b) can be computed.

Figure 5.

Surfaces representing $s^{\ast }(z,t)$ for Case C, $Pe=10$ (a) and $Pe=100$ (b). Note that the vertical scales of the left and right figures differ by a factor of 10. As time increases, the source term is exponentially damped. The magnitude of the source term is larger for increasing $Pe$.

8.1 Microscale concentration fields from numerical solution

Visualizations of the microscale concentration field at early times provide some direct evidence as to why studying Taylor dispersion at early times has been a challenging process. In figures 6 and 7, visualizations of the concentration field as it evolves from each of the three initial conditions are shown. To compare the results at different Péclet numbers, we have chosen the dimensionless time variable

(8.1)$$\begin{eqnarray}\unicode[STIX]{x1D70F}^{\ast }={\displaystyle \frac{t{\mathcal{D}}}{a^{2}}}Pe,\quad \text{or, equivalently, }\unicode[STIX]{x1D70F}^{\ast }={\displaystyle \frac{Ut}{a}}.\end{eqnarray}$$

This facilitates the direct comparison of plots that would, otherwise, have dramatically different time scales. The downside is that the actual time scale is somewhat obscured; we provide absolute times parenthetically to help maintain a feeling for the actual time scales involved. Some caution is necessary when interpreting these plots because the aspect ratio has been greatly increased for visualization purposes (i.e. the radial direction is magnified by a factor 10). In addition, to help with the visualization of the concentration at longer times (where the concentrations would be otherwise visually undetectable) the concentration field has been normalized and logarithmically transformed by $c^{\prime }=\log _{10}(c/c_{A0}+\unicode[STIX]{x1D700})$, where $\unicode[STIX]{x1D700}=0.1$, and $c_{A0}=\max [c(r,z,t)]$. For reference, the area-averaged concentrations for each case are presented to the right of the microscale concentration plots.

From figures 6 and 7, it is clear that the concentration evolution at early times is dominated by the particular initial configuration. Depending upon how the configuration is distributed across the velocity space, dramatically different kinds of behaviours can occur, and this is influenced by the relative importance of diffusion and convection as well as the local shear rate. It is useful to briefly discuss how this is related to the concept of mixing. In short, mixing is stretching-enhanced diffusion (Villermaux Reference Villermaux2019). The process of mixing in frequently divided into two conceptual components: (i) convective mixing (Lacey Reference Lacey1954) (or macromixing or stirring) (Villermaux Reference Villermaux2019), and (ii) diffusive mixing (or micromixing) (Epstein Reference Epstein1990; Bourne Reference Bourne2003).

From Newton’s law of viscosity the shear rate is given by (Bird, Stewart & Lightfoot Reference Bird, Stewart and Lightfoot2007)

(8.2)$$\begin{eqnarray}\dot{\unicode[STIX]{x1D6FE}}={\displaystyle \frac{\unicode[STIX]{x2202}v_{z}}{\unicode[STIX]{x2202}r}}={\displaystyle \frac{4Ur}{a^{2}}},\end{eqnarray}$$

where $\dot{\unicode[STIX]{x1D6FE}}$ is shear rate. Note that highest convective mixing occurs in places where shear rate is maximum (the region near the wall). Although the convective transport is highest at the centre of tube, it experiences the lowest shear rate and, consequently, lowest convection-mediated mixing. Radial diffusion conveys solute away from the centreline, creating diffusive mixing. More correctly, convection and diffusion create mixing in concert; shearing of the initial solute distribution ultimately creates a deformed configuration of the solute where diffusion is much more effective. Note that at small times for some of the initial configurations studied here (specifically Cases B and C), convection may actually impose conditions that transiently create less convective mixing before increasing again.

Even for seemingly simple initial conditions (e.g. Case A), we find that the early-time behaviour can be quite complex. For example, for $Pe=100$ at least three peaks are observable at $\unicode[STIX]{x1D70F}^{\ast }=15$ ($t=250$ min) (figure 7a,b the third peak occurs near $z=0.6~\text{m}$), even though there were only two peaks initially. At the beginning of the process, the concentration was uniform across the cross-section where the initial pulses were placed. Thus as time progresses, the concentration near the centre of the tube experiences more convection, whereas the solute located near the walls is transported mainly by diffusion. For Cases B and C, we find that the two initial peaks converge more rapidly for both Péclet numbers than for Case A; this is because the initial distribution on the left-hand side for these cases is distributed in the highest-velocity portion of the flow field (and the converse is true for the right-hand component of the initial condition). Thus, the centre of mass of the left-hand component catches up with the right-hand component. The effect of this is even more evident when we examine the behaviour of the moments of the solute. For $Pe=100$, by $\unicode[STIX]{x1D70F}^{\ast }=60$ ($t=1000~\text{min}$) we have essentially a single mode concentration field. This is a result, primarily, of the separation distance of the two components of the initial condition. Were they to have been separated by a greater distance, the time required to achieve a single modal concentration distribution in space would be longer.

8.2 Error analysis

In addition to issues of convergence, the numerical results also allow making estimates for the amount of error induced by the approximation made for the deviation balance equation. Specifically, we have imposed the following approximations in the analysis to this point:

(8.3a)$$\begin{eqnarray}\displaystyle & \displaystyle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}-\left\langle \tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\right\rangle \ll {\displaystyle \frac{{\mathcal{D}}}{r}}{\displaystyle \frac{\unicode[STIX]{x2202}}{\unicode[STIX]{x2202}r}}\left(r{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}r}}\right)-{\displaystyle \frac{{\mathcal{D}}}{r^{2}}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\tilde{c}}{\unicode[STIX]{x2202}\unicode[STIX]{x1D703}^{2}}}-{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}^{2}\tilde{c}}{\unicode[STIX]{x2202}z^{2}}}-\tilde{v}_{z}{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}, & \displaystyle\end{eqnarray}$$

(8.3b)$$\begin{eqnarray}\displaystyle & \displaystyle a\ll L_{0},\quad t^{\ast }\ll T^{\ast }. & \displaystyle\end{eqnarray}$$

$Pe(a/L_{0})\ll 1$

$a/L_{0}\ll 1$

$a/L_{0}\approx 1/20$

Therefore, the remaining questions regarding the error associated with the restriction given by the inequality (8.3a). This is best measured by the error observed between the upscaled model and the direct microscale numerical results. We can compute each of the terms in the inequalities in (8.3a)–(8.3b); however, the dimension of the result is as large as the numerical solution itself. To generate a reasonable summary metric, we propose to compute the following error (noting that $\widetilde{\tilde{v}_{z}\tilde{c}}=\tilde{v}_{z}\tilde{c}-\left\langle \tilde{v}_{z}\tilde{c}\right\rangle$ is the spatial deviation of the quantity $\tilde{v}_{z}\tilde{c}$).

(8.4)$$\begin{eqnarray}\unicode[STIX]{x1D716}_{1}(z,t)=\left({\displaystyle \frac{\langle |\widetilde{\tilde{v}_{z}\tilde{c}}|\rangle }{\left\langle |U\tilde{c}|+\left|{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}z}}\right|+\left|{\mathcal{D}}{\displaystyle \frac{\unicode[STIX]{x2202}\tilde{c}}{\unicode[STIX]{x2202}r}}\right|+|\tilde{v}_{z}\langle c\rangle |\right\rangle +\unicode[STIX]{x1D716}_{0}}}\times 100\right).\end{eqnarray}$$

Here, $\unicode[STIX]{x1D716}_{0}$ is a small number used only to assure that division by zero errors do not occur. A few plots of the metric $\unicode[STIX]{x1D716}_{1}(z,t)$ appear in the supplementary materials. This metric is still of high dimension, so to further reduce dimension (and generate a summary metric) we compute the first moment of $\unicode[STIX]{x1D716}_{1}(z,t)$ about the $z$-axis as follows:

(8.5a)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D716}_{closure}(t)={\displaystyle \frac{1}{A_{\unicode[STIX]{x1D716}}(t)}}\int _{z=-\infty }^{z=+\infty }{\displaystyle \frac{1}{2}}\unicode[STIX]{x1D716}_{1}^{2}(z,t)\,\text{d}z, & \displaystyle\end{eqnarray}$$

(8.5b)$$\begin{eqnarray}\displaystyle & \displaystyle A_{\unicode[STIX]{x1D716}}(t)=\int _{z=-\infty }^{z=+\infty }\unicode[STIX]{x1D716}_{1}(z,t)\,\text{d}z. & \displaystyle\end{eqnarray}$$

1. (i) The error of the approximation (8.3a) tends to increase as $Pe$ increases.

2. (ii) The error of the approximation decreases (not necessarily monotonically) with increasing time.

3. (iii) The observed error is influenced by the particular initial condition examined.

4. (iv) The maximum value of $\unicode[STIX]{x1D716}_{closure}$ for the $Pe=10$ case was less than 10 %, and the error rapidly decreased (within $\unicode[STIX]{x1D70F}^{\ast }<5$) to less than 5 %.

5. (v) The maximum value of $\unicode[STIX]{x1D716}_{closure}$ was of the order of 10 %–12 %; this was observed for $Pe=100$.

Overall, these results seem encouraging and reasonable. The comparison of the averaged result with the numerical results (described below) provide further evidence that the approximation is valid for the Péclet numbers considered here. For larger Péclet numbers, the error associated with the approximation given by (8.3a) tends to increase. For such cases, it may become necessary to solve the closure problems associated with $b$ and $\unicode[STIX]{x1D6F7}$ numerically without neglecting terms (an example of the numerical computation of $s^{\ast }$ is discussed in § 9 and in appendix A § A.6).

On the basis of the numerical results and the discussion above, it is possible to specify more useful constraints to increase the range of validity of the analysis. We suggest slightly more liberal constraints of the form

(8.6a)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D71B}Pe{\displaystyle \frac{a}{L_{0}}}=\boldsymbol{O}(1), & \displaystyle\end{eqnarray}$$

(8.6b)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{a}{L_{0}}}<1, & \displaystyle\end{eqnarray}$$

$\unicode[STIX]{x1D71B}$

$\unicode[STIX]{x1D71B}\approx 1$

$\unicode[STIX]{x1D71B}=1/2.2$

$\unicode[STIX]{x1D71B}=1/4$

$a/L_{0}\approx 1/10$

8.3 Computation using the upscaled balance equation

The upscaled problem given by (6.6a)–(6.6d) was solved as a one-dimensional model for the three initial condition cases. Note that the dispersion coefficient is independent of the initial condition, thus it remains identical for each case. Simulations were conducted using COMSOL in a manner consistent with what has been described in § 8.1 for the microscale simulations. The analytical solutions for $D^{\ast }$ and $s^{\ast }$ were computed using a custom-built code constructed in MATLAB; results were then imported into COMSOL, and interpolated to the grid using built-in routines. Simulations were assured to be convergent (using the approach described for the microscale simulations), and the average grid size was $1\times 10^{-4}~\text{m}$. Other solver parameters are identical to those reported in § 8.1 and table 2.

In figure 8, the averaged concentrations computed from (i) the numerical solution, and (ii) the upscaled, one-dimensional equation are compared. For $Pe=10$, the average concentration computed from the numerical solution is nearly indistinguishable from those predicted by the upscaled one-dimensional theory. We defined the following error metric for the averaged spatial concentration at a specified time, $t_{p}$ by

(8.7)$$\begin{eqnarray}\unicode[STIX]{x1D716}_{model}(t_{p},z)={\displaystyle \frac{|\langle c\rangle _{NS}-\langle c\rangle |}{\max (\langle c\rangle _{NS})}}\times 100,\end{eqnarray}$$

where the maximum in the denominator is taken as the maximum average concentration observed at time $t_{p}$. We computed the error from pairs of points separated by the minimum distance between the curves (as is done in computing total least squares) so that the error was not skewed by small displacement discrepancies. For the $Pe=10$ cases, the maximum error observed was less than 1.5 % for all times and all cases. For the $Pe=100$ cases, the maximum error was less than 7 % for all times and cases. For reference, plots of the errors are available in the supplementary materials. The correspondence between the two methods for computing the averaged concentration provide validation that the approximations given by (8.3a) and (8.3b) are reasonable for these Péclet numbers.

Figure 8.

Comparisons of the predictions of the average concentration. Profiles were computed by (i) averaging the microscale numerical simulations computed from (3.1a)–(3.1e) (denoted by NS), and (ii) numerically solving the averaged equation with the effective parameters $D^{\ast }$ and $s^{\ast }$ (equations (6.6a)–(6.7c)) (denoted by CSA). Results are for $Pe=10$ (a,c,e) and $Pe=100$ (b,d,f). The five fixed times are expressed in the dimensionless time variable $\unicode[STIX]{x1D70F}^{\ast }$.

8.4 Moment analysis

The spatial moments of the concentration field are frequently used to characterize the behaviour of the concentration field, both because of their appearance in the underlying theory, and because they provide information about the characteristics of the concentration distribution. The spatial moments in the $z$-direction of order $n$ ($n=0,1,2,3,\ldots$), $M_{n}$, are defined by

(8.8a)$$\begin{eqnarray}\displaystyle & \displaystyle M_{0}=\int _{z=-\infty }^{z=\infty }\int _{\unicode[STIX]{x1D703}=0}^{\unicode[STIX]{x1D703}=2\unicode[STIX]{x03C0}}\int _{r=0}^{r=a}c(r,\unicode[STIX]{x1D703},z,t)r\,\text{d}r\,\text{d}\unicode[STIX]{x1D703}\,\text{d}z, & \displaystyle\end{eqnarray}$$

(8.8b)$$\begin{eqnarray}\displaystyle & \displaystyle M_{n}(t)=\int _{z=-\infty }^{z=\infty }\int _{\unicode[STIX]{x1D703}=0}^{\unicode[STIX]{x1D703}=2\unicode[STIX]{x03C0}}\int _{r=0}^{r=a}z^{n}c(r,\unicode[STIX]{x1D703},z,t)r\,\text{d}r\,\text{d}\unicode[STIX]{x1D703}\,\text{d}z. & \displaystyle\end{eqnarray}$$

$n(n=0,1,2,3,\ldots )$

$\unicode[STIX]{x1D707}_{n}$

(8.9a)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D707}_{0}=M_{0}, & \displaystyle\end{eqnarray}$$

(8.9b)$$\begin{eqnarray}\displaystyle & \displaystyle \unicode[STIX]{x1D707}_{n}(t)={\displaystyle \frac{1}{\unicode[STIX]{x1D707}_{0}}}\int _{z=-\infty }^{z=\infty }\int _{\unicode[STIX]{x1D703}=0}^{\unicode[STIX]{x1D703}=2\unicode[STIX]{x03C0}}\int _{r=0}^{r=a}(z-M_{1}(t))^{n}c(r,\unicode[STIX]{x1D703},z,t)r\,\text{d}r\,\text{d}\unicode[STIX]{x1D703}\,\text{d}z. & \displaystyle\end{eqnarray}$$

(8.10)$$\begin{eqnarray}\unicode[STIX]{x1D707}_{2}(t)=\unicode[STIX]{x1D70E}^{2}(t)=M_{2}(t)-M_{1}^{2}(t)\end{eqnarray}$$

and the skewness, which is a normalized centred third moment, specified by

(8.11)$$\begin{eqnarray}\unicode[STIX]{x1D6FE}_{1}(t)={\displaystyle \frac{\unicode[STIX]{x1D707}_{3}(t)}{\unicode[STIX]{x1D707}_{2}^{3/2}(t)}}.\end{eqnarray}$$

In figures 9 and 10 we plot the second centred moment and the skewness as a function of time for each of the three initial conditions. One interesting feature that can be observed in these data is the distinct differences between the apparent time scales for the second centred moment and the skewness to attain their near-asymptotic behaviour. For the second moment, the asymptotic behaviour is represented by a linear increase in the moment with increasing $\unicode[STIX]{x1D70F}^{\ast }$; for the skewness, the asymptotic behaviour is the approach to a value of zero (cf. Chatwin Reference Chatwin1970). Examining the $Pe=10$ plots in figure 9, the slope of the second moment ($\text{d}\unicode[STIX]{x1D707}_{2}/\text{d}t$) reaches its asymptotic value for $\unicode[STIX]{x1D70F}^{\ast }$ near 2. The skewness, however, continues to show substantial evolution through the entire period plotted (up to $\unicode[STIX]{x1D70F}^{\ast }=60$). Similar kinds of behaviour can be observed for the $Pe=100$ data; the second moment is near asymptotic after approximately $\unicode[STIX]{x1D70F}^{\ast }=20$, whereas the skewness continues to evolve for the entire time period plotted. We have plotted the skew for both Péclet numbers on a log–log scale for a time interval up to $\unicode[STIX]{x1D70F}^{\ast }=300$ in figure 11; the long-time dynamics of the skew is more easily seen in that figure.

Figure 9.

Comparisons of the moments for different cases of the initial configuration for $Pe=10$. Moments were computed from two concentration fields as follows: (i) the microscale numerical simulations computed from (3.1a)–(3.1e) (denoted by NS), and (ii) the numerical solution of the averaged equation with the effective parameters $D^{\ast }$ and $s^{\ast }$ (equations (6.6a)–(6.7c)) (denoted by CSA).

Figure 10.

Comparisons of the moments for different cases of the initial configuration for $Pe=100$. Moments were computed from two concentration fields as follows: (i) the microscale numerical simulations computed from (3.1a)–(3.1e) (denoted by NS), and (ii) the numerical solution of the averaged equation with the effective parameters $D^{\ast }$ and $s^{\ast }$ (equations (6.6a)–(6.7c)) (denoted by CSA).

Figure 11.

Dynamics of the skewness for large values of $\unicode[STIX]{x1D70F}^{\ast }$. These results were computed directly from numerical simulations. The results represent Cases A, B and C for long-time evolution illustrating near-asymptotic behaviour not observable in figures 9 and 10. (a) $Pe=10$; (b) $Pe=100$. The approach to the asymptotic state is non-monotonic; from these solutions it is not possible to tell much more about the functional form of the approach.

For $Pe=100$, each of the three initial condition cases more obviously shows substantial transience in the skew. For each of the cases, the skewness starts at a negative value, and then crosses the zero to become positive. The approach to the asymptotic value then occurs slowly from the condition of positive skewness. Overall, these results indicate that skewness generally increases at early times, and this increase may ultimately lead to non-monotonic behaviour as the skewness approaches the asymptotic value. This is consistent with Chatwin (Reference Chatwin1970), who also found non-monotonic behaviour in third moment terms. Similar results can be seen in the $Pe=10$ cases (see the inset in figure 11a), although the time scales simulated do not allow a full analysis of the dynamics of the skewness at this value for $Pe$. Because our simulation times do not extend far enough, we cannot accurately assess the asymptotic behaviour of the skewness (such as those reported by Aris (Reference Aris1956) and Chatwin (Reference Chatwin1970)).

These results indicate that the approach to normality should not necessarily be measured by, for example, the approach of only the second moment to its asymptotic behaviour (i.e. achieving constant slope). While this is a useful metric, higher-order measures such as the skew may continue to show substantial evolution over a longer characteristic time scale indicating that the system as a whole is not necessarily near its asymptotic state of behaviour.

Figure 12.

Dynamics of the time derivative of the second moment for $Pe=100$. These results are obtained from the moments of the microscale numerical simulations computed from (3.1a)–(3.1e). The analytical solution produced by the upscaled theory is shown for comparison. Adopting the conventional definition of dispersion as $1/2\text{d}\unicode[STIX]{x1D707}_{2}/\text{d}t$ is not valid at early times for some initial conditions. In general, the definition based on $1/2\text{d}\unicode[STIX]{x1D707}_{2}/\text{d}t$ is only valid at asymptotic times. In contrast, the definition proposed using the upscaled theory presented is valid at all times and for all initial conditions.

8.5 Derivative of the second moment

In many theories of dispersion, the time derivative of the second moment is used to generate a de facto definition of the dispersion coefficient; usually, this is expressed in one dimension by

(8.12)$$\begin{eqnarray}D^{\unicode[STIX]{x1D707}_{2}}={\displaystyle \frac{1}{2}}{\displaystyle \frac{\text{d}\unicode[STIX]{x1D707}_{2}}{\text{d}t}}.\end{eqnarray}$$

Here, we have used the notation $D^{\unicode[STIX]{x1D707}_{2}}$ to distinguish this value from $D^{\ast }$. While such definitions are true asymptotically, they are not necessarily true for times that are near to the initial configuration time. One of the desirable traits for the dispersion coefficient identified in the Introduction is that it should be positive. This prevents conflicts with macroscale thermodynamics, and also assures that the resulting balance equations are well posed. However, there are initial configurations for which the second moment decreases in time before increasing again. This can be seen in the curves for $\unicode[STIX]{x1D707}_{2}$ (Cases B and C) for both $Pe=10$ and $Pe=100$ (figures 9 and 10). If one were to use the definition above then, for early times, a negative value for the dispersion coefficient would be produced. As an example, we have computed this quantity for $Pe=100$ and plotted it in figure 12. Note that for Case A, the definition for $D^{\unicode[STIX]{x1D707}_{2}}$ is identical to that defined for $D^{\ast }$; this is because $s^{\ast }$ is identically zero for that case. However, for the other two cases, we have an initial configuration that transiently reduces the second moment. This occurs because the initial configuration contains two parts: the first part (on the left) contains mass focused in the high-velocity regions, and is upstream from the second part. The second part (on the right) contains mass that is focused near the walls. The net result is that the centre of mass of the left part of the initial distribution moves faster than the right; thus, the left part eventually catches up to the right. This manifests physically as a decrease in the second moment. Thus the definition given by $D^{\unicode[STIX]{x1D707}_{2}}$ yields non-physical results for those cases because the effective dispersion coefficient is negative at some times; in contrast, $D^{\ast }(t)$ presented in (6.6a)–(6.7c) is strictly positive for all times.

These results provide some additional insight into the physical role of the $s^{\ast }$ field. Essentially, this field is a source term that assures that the spreading that is encoded by the initial configuration is correctly represented at early times. Because this is independent from the effective dispersion coefficient, there is no need to posit dispersion coefficients that, for example, violate macroscale thermodynamics by attaining negative values.

9.1 Macroscale dispersion: example 1

In order to isolate the effect of the $s^{\ast }$ field on the overall solution to the macroscale equations, we provide an example where its influence can be more readily understood. In this example, we illustrate that the conventional notion of superposition is still valid for the upscaled theory outlined previously.

For this example, a single solute injection is simulated as a sequence of two initial value problems. It is always possible to break initial value problems into parts like this when superposition is valid. The solution at the end of any one time interval is simply a concentration field; this concentration field can then be treated as the initial condition that is transported over a second time interval via the same balance equation.

For this example, we examine the transport of a single uniform pulse. We allow the initial condition to evolve until $t=T_{1}=250~\text{min}$. The solution at this time, $\langle c\rangle _{(t=T_{1},z)}$ is used to define the initial condition for the second time interval, $S_{2}$, at starting at$t^{\prime }=0~\text{min}$, and ending at $t^{\prime }=T_{\unicode[STIX]{x1D6E5}}=750~\text{min}$. The problem can be stated by the following sequence of two problems. The two problems can be written as

Time interval 1 solution $\quad S_{1}:0<t<250~\text{min}$

(9.1a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}=D^{\ast }(t){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}+{s_{1}}^{\ast }(z,t), & \displaystyle\end{eqnarray}$$

(9.1b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c\rangle |_{(z,t=0)}=c_{0}Z_{1}(z). & \displaystyle\end{eqnarray}$$

Time interval 2 solution $\quad S_{2}:0<t^{\prime }<750~\text{min}$

(9.1c)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t^{\prime }}}=D^{\ast }(t^{\prime }){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}+{s_{2}}^{\ast }(z,t^{\prime }), & \displaystyle\end{eqnarray}$$

(9.1d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.2}\quad \langle c\rangle |_{(z,t^{\prime }=0)}=\langle c\rangle |_{(z,t=T_{1})}. & \displaystyle\end{eqnarray}$$

Note that the second interval is written in terms of a new time variable, $t^{\prime }=t-T_{1}$ such that $0<t^{\prime }<T_{\unicode[STIX]{x1D6E5}}$. After the solution $\langle c\rangle |_{(z,t^{\prime })}$ is computed, it is straightforward to translate this solution to the original time variable via $t=t^{\prime }+T_{1}$.

The notable feature of this solution is that the dispersion coefficient has exactly the same dynamics for each of the two time intervals. To be explicit, recall $T_{1}=250~\text{min}$, and $T_{f}=1000~\text{min}$; the dispersion coefficients for the two intervals are given by

Interval 1 $\quad (0<t<250~\text{min})$

(9.2a)$$\begin{eqnarray}D^{\ast }(t)={\mathcal{D}}\left(1+{\displaystyle \frac{1}{48}}{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}\right)-4{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}}}\mathop{\sum }_{n=1}^{\infty }\left({\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\right)^{2}\exp \left(-\unicode[STIX]{x1D706}_{n}^{2}{\displaystyle \frac{{\mathcal{D}}}{a^{2}}}t\right).\end{eqnarray}$$

Interval 2 $\quad (0<t^{\prime }<750~\text{min})$

(9.2b)$$\begin{eqnarray}D^{\ast }(t^{\prime })={\mathcal{D}}\left(1+{\displaystyle \frac{1}{48}}{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}^{2}}}\right)-4{\displaystyle \frac{U^{2}a^{2}}{{\mathcal{D}}}}\mathop{\sum }_{n=1}^{\infty }\left({\displaystyle \frac{\text{J}_{3}(\unicode[STIX]{x1D706}_{n})}{\unicode[STIX]{x1D706}_{n}^{2}\text{J}_{0}(\unicode[STIX]{x1D706}_{n})}}\right)^{2}\exp \left(-\unicode[STIX]{x1D706}_{n}^{2}{\displaystyle \frac{{\mathcal{D}}}{a^{2}}}t^{\prime }\right).\end{eqnarray}$$

This means that $D^{\ast }(t=0)={\mathcal{D}}$ at the start of the first time interval, and that $D^{\ast }(t^{\prime }=0)={\mathcal{D}}$ at the start of the second time interval. For both intervals, the dispersion coefficient increases from its initial value with identical dependence upon time according to (9.2a) and (9.2b). In other words, there is no ‘memory’ for the dispersion coefficient.

We note that for the second time interval, the initial concentration field is not uniform in the radial direction; this means that the $s^{\ast }$ field is non-zero. This initial condition is also quite complex (i.e. it involves computing the $s^{\ast }$-field for the initial condition $\langle c\rangle |_{(z,t^{\prime }=0)}=c_{0}Z_{1}(z)+\langle c_{1}\rangle |_{(z,t=T_{1})}$), so there is no analytical solution for the $s^{\ast }$ field. Thus, $s^{\ast }$ is computed numerically, as described in § A.6. The $s^{\ast }$ field for the superposed initial condition at time $t^{\prime }=0~\text{min}$ is given in figure 13.

Figure 13.

Spatial and temporal dependence of the source term, $s^{\ast }$ for $Pe=100$ at $t^{\prime }=0~\text{min}$.

This example allows for a unique opportunity to directly assess the effect of the $s^{\ast }$ field. To do so, we consider the following three cases for obtaining a solution:

1. (i) The solution to the problem is determined by a single computation, spanning the interval $0\leqslant t\leqslant 1000~\text{min}$.

2. (ii) The solution is obtained for two time intervals, where the time intervals are given by $S_{1}:0\leqslant t\leqslant 750~\text{min}$ and $S_{2}:0\leqslant t^{\prime }\leqslant 750~\text{min}$. The $s^{\ast }$ field is computed as specified previously.

3. (iii) Strictly for comparison, the solution is obtained as the superposition of the two time intervals described above. The $s^{\ast }$ field, however, is set (incorrectly) to zero so that the solutions both with and without the $s^{\ast }$ field can be compared. This corresponds to the form of the time-dependent dispersion equation that is used frequently (cf. Sankarasubramanian & Gill (Reference Sankarasubramanian and Gill1973, equation (11))), and it exhibits the lack of time translation symmetry pointed out by Taylor (Reference Taylor1959).

The second moment is an effective measure for examining the result of these three cases. In figure 14 we have plotted the results of the solutions as computed for each of the three cases listed. In these results, we can consider the results from the first case (the black line in figure 14) to be the ground truth for comparison.

Figure 14.

Two-step process for $Pe=100$. (i) Case 1. The solution solved over the whole (1000 min) time period. (ii) Case 2 (first step). The solution, $S_{1}$, for $0<t<250~\text{min}$. (iii) Case 2 (second step) The solution, $S_{2}$ for $0<t^{\prime }<750~\text{min}$ ($250<t<1000~\text{min}$) with the source term computed numerically, and illustrated in figure 13. (iv) Case 3. The solution, $S_{2}$ for $0<t^{\prime }<750~\text{min}$ with $s^{\ast }=0$.

We note that, for the solution computed in two steps with the correct value for $s^{\ast }$, the second moment is continuous, and it matches the single-step solution almost identically. This occurs even though the dispersion coefficient returns to its zero-time value when the problem is restarted at time $t=250~\text{min}$. This behaviour occurs because of the unique interplay between the effective dispersion coefficient, $D^{\ast }$, and the source term given by $s^{\ast }$. Thus, the concern posed by Taylor (Reference Taylor1959) about the paradox of which dispersion coefficient to use (the one at the end of the first time interval, or the one corresponding to zero elapsed time for the second time interval) does not arise. The dispersion coefficient is unequivocally defined for both time periods by (9.2a)–(9.2b), and superposition of the solutions for the two time intervals leads to a solution that contains no discontinuities in the slope of the second moment.

For Case 3, we note that without the proper $s^{\ast }$ field correction, the second moment develops a cusp at $t=250~\text{min}$. In other words, the rate of spreading for the second time interval is too small, and this occurs because the source term $s^{\ast }$ has been neglected. This creates a technical problem, because the derivative of the second moment does not exist at that point. Additionally, the second moment then grows too slowly for the remaining time, under-predicting the actual value significantly.

This case not only allows a comparison to better illustrate how the $s^{\ast }$ field influences the solution to account for the initial distribution of matter, but it helps to resolve the apparent paradox that troubled Taylor (Reference Taylor1959). Specifically, for dispersion in tubes, the dispersion process is not independent of the initial condition at early times; however, this dependence is best represented through $s^{\ast }$ rather than $D^{\ast }$. For initial conditions that are uniform in the radial direction, no additional modification from conventional theory is needed. However, for initial conditions that are not uniform in the radial direction, the initial condition itself generates a behaviour that is accounted for by the appearance of the non-conventional source term $s^{\ast }$ in the macroscale transport equation. The inclusion of the additional source term is essential for predicting the correct macroscale dynamics of the system.

9.2 Macroscale dispersion: example 2

In this example, we illustrate through direct deviation and computation that our solution is superposable in the sense that was desired by Taylor (Reference Taylor1959). For this problem, the system starts with a specified initial condition and progresses for some time ($0<t<T_{1}$). Then, a second source is instantaneously injected into the system, and transport continues over the interval $T_{1}<t<T_{f}$. This situation, then, yields a condition where two solutes are in the system for varying amounts of time (and, hence, would experience different time-dependent effective diffusion coefficients). Taylor’s Reference Taylor1959 concern was the logical incongruity associated with assigning two different values of the dispersion coefficient at the same point where the solute bodies overlap. In the following, we show that the framework developed above avoids this problem.

9.2.1 The superposition problem for a two release case

This example is much like example 1, except now we consider the case where there are two injections of solute at two different times. This represents exactly the conditions that which were addressed by Taylor (Reference Taylor1959). In other words, the case of two releases leads to the problem where two solute distributions, each having been in the system for different amounts of time, might overlap. The conventional approach (e.g. Sankarasubramanian & Gill (Reference Sankarasubramanian and Gill1973, equation (11))) using a time-dependent dispersion coefficient (without a source term for correction) would lead to a problem where two different values of the dispersion coefficient would occur at points where the solute distributions overlapped. In this example, we illustrate that the balance equation for the average concentration that we derive can be sensibly superposed.

To start the discussion, we first need to determine mathematically how to handle a second pulse injected at some time $t=T_{1}$ after progression from a defined initial condition at $t=0$. The sudden injection of solute into the system at $t=T_{1}$ introduces a discontinuity of the solute field in time. Although there are several ways that this might be represented, the simplest one is to use superposition in the following way. For the first time interval ($0<t<T_{1}$), the system evolves from the specified initial condition (for these examples, we will use the function $Z(z)$ defined previously in (7.11a), such that $\langle c\rangle |_{(z,t=0)}=c_{0}Z_{1}(z)$). At time $t=T_{1}$, a new solute source is instantaneously injected into the system. The new initial condition for the second time interval is then the superposition of the second pulse configuration with the configuration of the existing solute distribution field, $\langle c\rangle |_{(z,T_{1})}$. This new field forms an initial condition for the second time interval, beginning at time $t=T_{1}$ and ending at time $t=T_{f}$. In the comments by Taylor (Reference Taylor1959), this is ostensibly what is meant by the use of the word ‘superposition’. Thus, we consider two problems that together provide the necessary solution.

To make this concrete, again let $T_{1}=250~\text{min}$ and $T_{f}=1000~\text{min}$. The two problems can be written as follows. We define the associated independent transport equations for the solute injections (indicated by $I_{1}$ and $I_{2}$) for the entire time interval ($0<t<1000~\text{min}$) to be described by

Problem $\langle c_{1}\rangle \quad I_{1}:0<t<1000~\text{min}$

(9.3a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}t}}=D^{\ast }(t){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z}}+{s_{1}}^{\ast }(z,t), & \displaystyle\end{eqnarray}$$

(9.3b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c_{1}\rangle |_{(z,t=0)}=c_{0}Z_{1}(z). & \displaystyle\end{eqnarray}$$

Problem $\langle c_{2}\rangle \quad I_{2}:0<t^{\prime }<750~\text{min}$

(9.3c)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{2}\rangle }{\unicode[STIX]{x2202}t^{\prime }}}=D^{\ast }(t^{\prime }){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c_{2}\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{2}\rangle }{\unicode[STIX]{x2202}z}}+{s_{2}}^{\ast }(z,t^{\prime }), & \displaystyle\end{eqnarray}$$

(9.3d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.2}\quad \langle c_{2}\rangle |_{(z,t^{\prime }=0)}=c_{0}Z_{1}(z). & \displaystyle\end{eqnarray}$$

For the second injection, the time coordinate for the second interval is started at the time $t^{\prime }=t-T_{1}$, as described in example 1. Without this translation, the second injection would not start with the correct dispersion coefficient, which is $D^{\ast }(t^{\prime }=0)={\mathcal{D}}$, as indicated by (9.2b).

The boundary conditions are identical to those posed in (3.1a)–(3.1e). For reference, the microscale solution to this problem is provided for a number of time points in figure 15. We note that problem $\langle c_{2}\rangle$ must be put in the time coordinates for which the injection happens at time equal to zero (this was noted in § 7.2) to properly define $D^{\ast }$ and $s^{\ast }$.

Figure 15.

Microscale solute distributions in space at selected time points for the problem consisting of two injected pulses; Péclet number is $Pe=100$. The second pulse is injected at the same location where the first pulse was injected at $t=250~\text{min}$. These images are provided only for visualization of the microscale processes (aspect ratio is 1 : 10 as for figures 6 and 7), and for validation of the macroscale equations by comparison of the directly averaged microscale fields.

We now explore how these two solutions can be superimposed. First, note that the classical principle of superposition (Polyanin Reference Polyanin2000; Olver Reference Olver2014) for linear partial differential equations with time-dependent coefficients requires that the superposition be defined over the same time interval. Thus, problems $I_{1}$ and $I_{2}$ can be equivalently written as (recalling that for the general problem, the initial condition is represented by $\unicode[STIX]{x1D711}(z)$; cf. (3.1e))

Problem $\langle c_{1}\rangle \quad I_{1}:0<t<1000~\text{min}$

Interval 1 $\quad 0<t<250~\text{min}$

(9.4a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}t}}=D^{\ast }(t){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z}}+{s_{1}}^{\ast }(z,t), & \displaystyle\end{eqnarray}$$

(9.4b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c_{1}\rangle |_{(z,t=0)}=c_{0}Z_{1}(z). & \displaystyle\end{eqnarray}$$

Interval 2 $\quad 0<t^{\prime }<750~\text{min}$

(9.4c)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}t^{\prime }}}=D^{\ast }(t^{\prime }){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{1}\rangle }{\unicode[STIX]{x2202}z}}+{s_{1}}^{\ast }(z,t^{\prime }), & \displaystyle\end{eqnarray}$$

(9.4d)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.2}\quad \langle c_{1}\rangle |_{(z,t^{\prime }=0)}=\underbrace{\langle c_{1}\rangle |_{(z,t=T_{1})}}_{\unicode[STIX]{x1D711}_{1}}. & \displaystyle\end{eqnarray}$$

Problem $\langle c_{2}\rangle \quad I_{2}:0<t<1000~\text{min}$

Interval 1 $\quad 0<t<250~\text{min}$

(9.4e)$$\begin{eqnarray}\langle c_{2}\rangle =0.\end{eqnarray}$$

Interval 2 $\quad 0<t^{\prime }<750~\text{min}$

(9.4f)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{2}\rangle }{\unicode[STIX]{x2202}t^{\prime }}}=D^{\ast }(t^{\prime }){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c_{2}\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c_{2}\rangle }{\unicode[STIX]{x2202}z}}+{s_{2}}^{\ast }(z,t^{\prime }), & \displaystyle\end{eqnarray}$$

(9.4g)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.2}\quad \langle c_{2}\rangle |_{(z,t^{\prime }=0)}=\underbrace{c_{0}Z_{1}(z)}_{\unicode[STIX]{x1D711}_{2}}. & \displaystyle\end{eqnarray}$$

We make the following important notes about the formulation above.

(i) We have divided Problem 1 into two intervals $0<t<250~\text{min}$ and $250<t<1000~\text{min}$. This is not an arbitrary choice; it is necessary to obtain solutions that involve multiple initial conditions.

(ii) In our formulation, the dispersion coefficient $D^{\ast }$ does not have to ‘remember’ its prior history. Hence, exactly the same function $D^{\ast }$ is used in both intervals. Being explicit, for the problem for $\langle c_{1}\rangle$ in the first time interval, the dispersion coefficient starts at $D^{\ast }(t=0)={\mathcal{D}}$, and grows as predicted by (7.3). When time is restarted in the second interval, exactly the same behaviour is repeated. The dispersion coefficient for the second time interval starts at $D^{\ast }(t=0)={\mathcal{D}}$, and again grows as predicted by (7.3). During the second time interval, the source function $s_{1}^{\ast }$ automatically accounts for the spreading inherent in the second initial condition. This function is essentially the ‘memory’ in the system, but one that encodes that memory in a local rather than non-local in time representation.

(iii) The source function, $s^{\ast }$, is linear in the initial condition; this is proved in § A.5. In other words, we have the following decomposition due to linearity:

(9.5)$$\begin{eqnarray}s^{\ast }(\unicode[STIX]{x1D711}_{1}+\unicode[STIX]{x1D711}_{2})=s^{\ast }(\unicode[STIX]{x1D711}_{1})+s^{\ast }(\unicode[STIX]{x1D711}_{2}).\end{eqnarray}$$

(iv) These features make the two problems superposable; the two problems can be added to generate one equation that suffices to describe the dispersion process over the two intervals.

9.2.2 Superposition of the two concentrations

We now show how superposition can be accomplished for the problem of two releases of solute at two different times. We begin by defining the superposed concentration $\langle c\rangle =\langle c_{1}\rangle +\langle c_{2}\rangle$. For the first time interval, the superposition is trivial, noting that $\langle c_{2}\rangle \equiv 0$. Thus, $\langle c\rangle =\langle c_{1}\rangle$. Superposition for the first interval yields

Superposition for interval 1 $\quad 0<t<250~\text{min}$

(9.6a)$$\begin{eqnarray}\displaystyle & \displaystyle {\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t}}=D^{\ast }(t){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}+{s_{1}}^{\ast }(z,t), & \displaystyle\end{eqnarray}$$

(9.6b)$$\begin{eqnarray}\displaystyle & \displaystyle \text{I.C.1}\quad \langle c\rangle |_{(z,t=0)}=c_{0}Z_{1}(z). & \displaystyle\end{eqnarray}$$

Note that the concentration at the final time $t=T_{1}=250~\text{min}$, forms the initial condition for $\langle c_{1}\rangle$ during the second interval. For reference, we denote this concentration by $\langle c_{1}\rangle |_{(z,t=T_{1})}$.

Because (9.4d) and (9.4g) are (i) linear, and (ii) defined over the same time interval $0<t^{\prime }<(T_{f}-T_{1})$, the superposition of these equations is straightforward. Adding (9.4c) and (9.4f) yields

Superposition for interval 2 $\quad 0<t^{\prime }<750~\text{min}$

(9.6c)$$\begin{eqnarray}{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}t^{\prime }}}=D^{\ast }(t^{\prime }){\displaystyle \frac{\unicode[STIX]{x2202}^{2}\langle c\rangle }{\unicode[STIX]{x2202}z^{2}}}-U{\displaystyle \frac{\unicode[STIX]{x2202}\langle c\rangle }{\unicode[STIX]{x2202}z}}+s^{\ast }(z,t^{\prime }).\end{eqnarray}$$

Here, we have used the linearity of the source term: $s^{\ast }(z,t^{\prime };\unicode[STIX]{x1D711})=s_{1}^{\ast }(z,t^{\prime };\unicode[STIX]{x1D711}_{1})+s_{2}^{\ast }(z,t^{\prime };\unicode[STIX]{x1D711}_{2})$ to generate the single source term field, $s^{\ast }$, for the superposed problem. The initial condition for the second interval is found by adding the final concentration from time interval 1, $\langle c_{1}\rangle |_{(z,t=T_{1})}$, to the initial condition for the second solute release.

(9.6d)$$\begin{eqnarray}\text{I.C.2}\quad \langle c\rangle |_{(z,t^{\prime }=0)}=\underbrace{\langle c_{1}\rangle |_{(z,t=T_{1})}+c_{0}Z_{1}(z)}_{\unicode[STIX]{x1D711}}.\end{eqnarray}$$

The Taylor dispersion problem is frequently represented by an equation of the form of (9.4d) and (9.4g), but with $s_{1}^{\ast }=s_{2}^{\ast }=0$ (cf. Smith Reference Smith1981a). Superposition for this case fails because even if one divides the problem into two time intervals. Upon restarting time (setting $t^{\prime }=0$) for the second interval, the concentrations $\langle c_{1}\rangle$ and $\langle c_{2}\rangle$ are represented by two different linear operators (one for $\langle c_{1}\rangle$ where $D^{\ast }(t)$ begins at $t=T_{1}$, and a second for $\langle c_{2}\rangle$ where $D^{\ast }(t^{\prime })$ begins at $t^{\prime }=0$). In the formulation we provide, $D^{\ast }(t)$ is always given by a single function of time everywhere in the domain; any ‘time history’ associated with multiple injections at different times is accounted for strictly through the source term field, $s^{\ast }$. This avoids the possibility of having $D^{\ast }$ being multi-valued at a single spatial location.

9.2.3 Proof of validity of superposition by direct computation

The superposition of $\langle c_{1}\rangle$ and $\langle c_{2}\rangle$ is given by (9.6a)–(9.6d). For clarity, we re-emphasize the following regarding the interpretation of these equations:

1. (i) During the first time interval ($0<t<T_{1}$) the dispersion coefficient for the time interval starts at $D^{\ast }(t=0)={\mathcal{D}}$, and again grows as predicted by (7.3). This is described by the single transport equation given by (9.6a,b). Because the radial derivative of the initial condition for this interval is zero, we have that $s_{1}^{\ast }(z,t)$ is zero.

2. (ii) For the second time interval, the initial condition is the solution obtained from the end of the first time interval (at $t=T_{1}$) plus the initial condition representing the second solute release. This is described by the single transport equation given by (9.6c,b).

3. (iii) During the second time interval ($0<t<T_{1}$) the dispersion coefficient for the time interval starts at $D^{\ast }(t=0)={\mathcal{D}}$, and again grows as predicted by (7.3). Note that the radial derivative of the initial condition for the second time interval is non-zero, thus there is a contribution from the $s^{\ast }$-field for the second time interval.

The initial condition for this problem is similar to that for Problem 1. In fact, the $s^{\ast }$ field is identical to that for Problem 1, and is computed numerically as described for Problem 1.

Figure 16.

The macroscopic concentration field predicted by the upscaled problem statements given by $I_{1}$ and $I_{2}$. Continuous lines represents the averaged microscale simulation results; points represent the solutions to the upscaled equations given by (9.3a)–(9.3d). The concentration curves are provided as two plots for ease in visualization. Note that the curve in dark blue at $t=250~\text{min}$ represents the macroscale initial condition for problem $I_{2}$ computed by superposition.

In figure 16 we have illustrated the solutions for this problem computed by (i) averaging the microscale numerical solutions directly, and (ii) via the two-step (superposed) macroscale simulation (solving (9.6a)–(9.6d)) as described above. We note that the two solutions are in good agreement, and, in particular, the amount of dispersion predicted by the upscaled model (both before and after the second pulse) is consistent with the averaged microscale data (for which there are no approximations of any kind). There is a slight mismatch in between the two solutions near the peaks for times $t=100$, 350 and 500 min. Most likely, these errors are associated with the approximations in the upscaled equation, as discussed previously (cf. the peaks for $Pe=100$, Case A in figure 8).

In summary, we have provided two examples that meet the desideratum of Taylor (Reference Taylor1959). For each solution, we find that (i) we can define a sensible notion of superposition for the upscaled equation of the form that we have derived, (ii) the associated dispersion coefficient is always a single-valued function of space and (iii) the source terms are superposable, and they generate a field correction that assures that the proper rate of spreading (or, equivalently, second moment) is achieved. Because the source terms are responsible for correcting the rate of spreading at early times, this function is not imposed on the dispersion coefficient. It is this component of our solution that generates the necessary conditions for the upscaled equation to be superposable.