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Natural frequency discontinuity of vertical liquid sheet flows at transcritical threshold

Published online by Cambridge University Press:  28 July 2022

Matteo Chiatto*
Affiliation:
Department of Industrial Engineering, Università di Napoli “Federico II”, Naples 80125, Italy
Alessandro Della Pia
Affiliation:
Department of Industrial Engineering, Università di Napoli “Federico II”, Naples 80125, Italy
*
Email address for correspondence: matteo.chiatto@unina.it

Abstract

The natural and forced dynamic response of a gravitational plane liquid sheet (curtain) of finite length interacting with an unconfined gaseous ambient is numerically and experimentally investigated. The global eigenvalue spectrum obtained by means of a linear inviscid one-dimensional model, accounting for the coupling between the curtain motion and the ambient pressure disturbances, clearly shows an abrupt increase (jump) in the characteristic natural frequency of the flow when the supercritical ($We>1$) to subcritical ($We<1$) transition occurs, with the Weber number $We$ defined as the ratio between inertia and capillary forces. On the other hand, the numerical simulation of the forced sheet response does not show any discontinuity between supercritical and subcritical conditions, as recently found by Torsey et al. (J. Fluid Mech., vol. 910, 2021, pp. 1–14) in the case of an infinite liquid sheet subjected to imposed ambient pressure disturbances not coupled with the curtain motion. It is argued that the forced liquid sheet behaviour varies continuously in shape and amplitude between the two regimes, not depending on the specific liquid–gas interaction model considered, whilst the natural frequency of the finite flow system does undergo a discontinuity, which can be theoretically predicted by the model of sheet–ambient interaction employed here. As a major result, the experimental evidence of the natural frequency jump is for the first time provided as well.

Information

Type
JFM Papers
Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduction, provided the original article is properly cited.
Copyright
© The Author(s), 2022. Published by Cambridge University Press.
Figure 0

Figure 1. Schematic representation of (harmonically forced) liquid sheet.

Figure 1

Figure 2. Sketch of the experimental apparatus. Details of the two-dimensional liquid sheet and the nozzle are reported on the right. The red spot in the sheet plane denotes the measuring point.

Figure 2

Figure 3. Combined $We$$Fr$ effect on the eigenvalues (a,b) and on the normalized least stable eigenfunction, (c): $(We,Fr)$ = $(1.2,0.08)$, black filled dot and continuous black line; $(1.05,0.07)$, black open dot and dashed black line; $(0.95,0.06)$, red filled dot and continuous red line; $(0.8,0.05)$, red open dot and dashed red line.(b) Shows a zoom of the inner parts of the spectra reported in (a). The characteristic frequencies ${\rm \Delta} \lambda ^{+}_i$ and ${\rm \Delta} \lambda ^{-}_i$, whose values are listed in table 2, are indicated respectively in (a,b).

Figure 3

Table 1. Dimensionless parameters involved in the numerical analysis.

Figure 4

Table 2. Global frequency in supercritical (${\rm \Delta} \lambda ^{-}_i$, $We>1$) and subcritical (${\rm \Delta} \lambda ^{+}_i$, $We<1$) flow regimes.

Figure 5

Figure 4. Weber number effect on the sheet centreline deflection, $\ell$, as a function of the streamwise station, $x$, at different fractions of oscillation period $T$: $t=0 T$ (black); $0.25 T$ (red); $0.5 T$ (blue); $0.75 T$ (green). The dashed line denotes the centreline of the unperturbed curtain. From top to bottom: $f^{\star } = 1, 5$ and $20$ Hz.(a) $(We, f^{\star })=(1.05, 1\,\text {Hz})$; (b) $(We, f^{\star })=(0.95, 1\,\text {Hz})$; (c) $(We, f^{\star })=(1.05, 5\,\text {Hz})$; (d) $(We, f^{\star })=(0.95, 5\,\text {Hz})$; (e) $(We, f^{\star })=(1.05, 20\,\text {Hz})$; ( f) $(We, f^{\star })=(0.95, 20\,\text {Hz})$.

Figure 6

Figure 5. Normalized power spectral density of the vibrometer recordings acquired at different values of the Weber number.

Figure 7

Figure 6. Comparison between numerical ($\,f^{\star }_{n}$, continuous curves) and experimental ($\,f^{\star }_{e}$, filled circles) natural frequencies in supercritical (black) and subcritical (red) regimes. The numerical frequency associated with the fast branch of the spectrum in supercritical conditions is also reported (black dashed curve). The error bars represent the standard deviation of the experimental measurements.

Figure 8

Table 3. Experimental and numerical values of the natural frequency varying the Weber number. The relative percentage spread $\epsilon$ is defined as $\epsilon = 100 \cdot (f^{\star }_{n} - f^{\star }_{e})/f^{\star }_{n}$. The last column reports the standard deviation of the experimental measurements.

Figure 9

Figure 7. Eigenvalue spectrum (a), ${\rm \Delta} \lambda ^{-}_i$ (b) and curtain natural characteristic frequency $f^{\star }_n$ (c) varying the Froude number. In (b,c), both the theoretical predictions (continuous black curve) and the numerical evaluations from the spectrum (black circles) are reported. Here, $We=1.2$.

Figure 10

Figure 8. Analysis of the curtain natural characteristic frequency $f^{\star }_n$ in the limit case of $Fr \to 0$ in supercritical (a) and subcritical (b) conditions. The dimensionless values ${\rm \Delta} \lambda ^{\pm }_i$ are also reported (c,d).

Figure 11

Figure 9. Weber number effect on the sheet centreline deflection, $\ell$, as a function of the streamwise station, $x$, at different fractions of oscillation period $T$: $t=0 T$ (black); $0.25 T$ (red); $0.5 T$ (blue); $0.75 T$ (green). Results of the numerical integration of (B1)–(B2) (continuous curves); (B3)–(B4) (dotted curves). The dashed line denotes the centreline of the unperturbed curtain. From top to bottom: $f^{\star } = 1, 5$ and $20$ Hz.(a) $(We, f^{\star })=(1.05, 1\,\text {Hz})$; (b) $(We, f^{\star })=(0.95, 1\,\text {Hz})$; (c) $(We, f^{\star })=(1.05, 5\,\text {Hz})$; (d) $(We, f^{\star })=(0.95, 5\,\text {Hz})$: (e) $(We, f^{\star })=(1.05, 20\,\text {Hz})$; ( f) $(We, f^{\star })=(0.95, 20\,\text {Hz})$.