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“Once you have done your homework you realize we need new politics, we need new economics … We need a whole new way of thinking.”
Greta Thunberg, speech at EESC event “Civil Society for rEUnaissance”
There were fortunes to be made in coal and then oil, and now gas too. More than just fortunes are involved; modern economies depend on these fuels, and states only function if fuels are available to keep modern life going. Access to fuel has been essential to the security of modern states and their inhabitants. The rivalries of states and corporations, the struggles for dominance and control, the political arguments about who has access to what where matters. In other words, geopolitics are indivisible from fossil fuels in the modern world. Other resources have been involved in all sorts of conflict and imperial plunder through history (LeBillon 2012), but oil has pride of place in recent decades.
A sustainable future now requires dismantling these systems and replacing both the technologies and their social and economic arrangements with ones fit for a small vulnerable biosphere. No longer can assumptions of a big world as a stage for geopolitics operate if the long-term future of humanity is to be secured. Numerous peoples have long paid a high price for the struggles for power and space set in motion by European colonization and the expansion of capitalism through the Earth system (Grove 2019). Now even those who have benefited most from these colonial arrangements and their subsequent evolution into the global economy are beginning to feel the impacts of sea-level rise and climate disruption.
The large oil companies are truly global companies with holdings and infrastructure in many countries. Crucially in many places they held the rights to exploit petroleum and their wealth was tied to the valuations of these reserves. This is often still the case and stock values are linked directly to gaining access to what lies deep underground. States have struggled to exploit these resources and enrich themselves in the process too. The case of the Gulf States, sheikdoms sitting on oil fields, emphasizes the point that there are vast fortunes to be made. But fuel resources are unevenly spread around the globe, and while some states and corporations have gained enormous wealth others have had economic disruptions because of their dependence on fuel from abroad.
“People know what they do; they frequently know why they do what they do; but what they don't know is what what they do does.”
Michel Foucault, Madness and Civilization
The Promethean moment
Since life first emerged from oceans and plants started growing on land surfaces fires have had fuel. It's so obvious that we don't often think about it, but stuff that was once living is what burns. Trees provide firewood. The paper we use to start fires in our coal or wood burning stoves comes from trees. If we use fire starters instead of paper most of them are petroleum based. And petroleum is in fact a deeply buried residue of former life.
Mostly we burn fossil fuels. Coal, petroleum and natural gas all come from the remains of decayed living things. Organic material, stuff that was once living, has lots of carbon in it, and burning it produces carbon dioxide gas. Once it collects in the atmosphere it traps heat and warms the world. Oxygen is a by-product of life too, and it is also what is needed to make fire. That and a spark to start a flame so that the process of combining the carbon from organic stuff, things that were once alive, with oxygen in the air, can happen.
We will never know exactly how the human use of fire started, but it is a reasonable guess that it started in various places in different ways. What matters, as fire historian Steven Pyne (2021) makes very clear, is that, unlike any other species we learned to start fires. Yes, we have language, and culture, and tools, and religions and lots of other things that we think separate us from other species. But beavers are great hydrological engineers; elephants have complicated communication systems; whales too. Ants and other insects build complex structures. Only us humans start fires.
Once we learned that “ignition trick” in Pyne's apt phrase, we could have fires pretty much where and when we wanted them. It is difficult in the rain for sure and fires are hard in a desert or on Arctic ice sheets, far from plants to use for fuel. But nonetheless we could have heat where we needed it much of the time, and that made a difference, a very big one as it turned out.
“We got small guts and big heads because we could cook food. We went to the top of the food chain because we could cook landscapes. And we have become a geologic force because our fire technology has so evolved that we have begun to cook the planet.”
Stephen Pyne, “The Fire Age”
It would be a mistake to argue that fire explains all human history. It is not the only thing we need to focus on in trying to think through the implications of the Anthropocene for how we need to live in coming decades. Other things matter too: culture, politics and the new innovations of digital technologies. But when you dig into these other aspects of human accomplishment, somewhere in there fire has historically played a key role.
We are an urban species now; the majority of us live in cities and towns, and even those of us who don't live in cities rely on all sorts of things that urban civilization provides. Humans live scattered all over the planet, mostly on land, although a few of us are on the water on in the air at any one given moment! But wherever we live we rely on cooked food for our subsistence, and until the invention of microwaves, cooking relied on an external source of heat, and most of that heat was a matter of fire of some form or other.
Food is key to cultural life for most of us. Kitchens have stoves, and these places are key to social life. Fireplaces in many homes have long been the source of heat, the focus of family life. Hearth and home go together. Rituals of food preparation, family recipes and shared meals are all tied into the apparatus of heating to cook food. Cooking, as Stephen Pyne puts it, has changed us in numerous ways because it has dramatically altered what we can digest, allowing us, unlike most other species, to become omnivorous, able to eat all sorts of things.
Simple fires offer warmth and the ability to cook food. These two key parts of human life have effectively been moved from our bodies to the surrounding habitat. Our digestions are extended by cooking, allowing us to eat things from which we would otherwise have trouble gaining nourishment.
Fluid flow passing a post-buckled sheet placed between two close confining walls induces periodic snap-through oscillations and contacts that can be employed for triboelectric energy harvesting. The responses of a two-dimensional sheet to a uniform flow and wall confinement in both equilibrium and post-equilibrium states are numerically investigated by varying the distance between the two ends of the sheet, gap distance between the confining walls and flow velocity. Cases with strong interactions between the sheet and walls are of most interest for examining how contact with the walls affects the dynamics of the sheet and flow structure. At equilibrium, contact with the wall displaces the sheet to form a nadir on its front part, yielding a lower critical flow velocity for the transition to snap-through oscillations. However, reducing the gap distance between the walls below a certain threshold distinctly shifts the shape of the sheet, alters the pressure distribution and eventually leads to a notable delay in the instability. The contact between the oscillating sheet and the walls at post-equilibrium is divided into several distinct modes, changing from sliding/rolling contact to bouncing contact with increasing flow velocity. During this transition, the time-averaged contact force exerted on the sheet decreases with the flow velocity. The vortices generated at the extrema of the oscillating sheet are annihilated by direct contact with the walls and merging with the shear layers formed by the walls, resulting in a wake structure dominated by the unstable shear layers.
Stephen Pyne's (2015, 2021) accounts of fire history show that we have been changing the way we engineer fire. From the early days of open fires, we added furnaces for smelting, fireboxes for steam engines, and then the pistons and cylinders of internal combustion engines. All of these are about constraining and controlling the forces of combustion to make it serve our needs. Recently we have added fire engines, hoses, and preventative measures in terms of building codes, sprinkler systems, and fire hydrants to city streets too so we can better deal with things when they burn where they should not. Now we need to constrain fire still further so that we can control the large-scale consequences of our use of combustion. If we do so, in turn we will have a better chance of tackling the wildfires.
Can we, as Naomi Klein (2014) suggested a decade ago, reimagine our cities in ways that take their energy consumption seriously and allow us to regain control of it from fossil fuel companies? Some cities and municipalities, faced with rising tides, damage from storms and citizens demanding action, are starting to declare states of climate emergency. They are beginning to think long and hard about how to both adapt to changes that are unavoidable, and act in ways that don't make things even worse. Can industrial societies also curtail the exploitation of resources from the lands of conquered peoples, and in the process rebuild energy systems that can give them economic futures and a life within their ecological contexts? This should help with the extinction crisis that we all face.
Reworking our financial institutions to invest in sensible buildings, energy systems that do not require burning things, and remaking cities that are much healthier both because they have less pollution and can better cope with extreme weather, is a future worth working hard for; the Greta Thunberg generation deserve no less. Babcock Ranch in Florida, the community designed to run on solar power and to deal with extreme weather, which survived Hurricane Ian in 2022, points the way to building and planning sensibly for a climate-disrupted future.
The field of research related to CO2 capture is significant and really attractive for sustainable green chemistry. Focusing attention on this topic in our research led to obtaining new compounds based on diamines. As a result of the syntheses carried out using aqueous solutions of diamines exposed to the slow action of carbon dioxide from the air, three new monocarbamates were obtained. X-ray powder diffraction data for the obtained compounds: 12-propCO2 (C4H10N2O2) [a = 9.3033(7), b = 9.2485(7), c = 7.4735(7) Å, β = 111.214(7)°, V = 599.46 Å3, Z = 4, space group Ia]; 13-propCO2 (C4H10N2O2) [a = 5.0065(10), b = 12.2093(23), c = 4.9006(10) Å, β = 96.457(18)°, V = 297.65 Å3, Z = 2, space group P21]; and 13-dytekCO2 (C6H14N2O2) [a = 28.374(3), c = 5.1726(9) Å, V = 3606.53 Å3, Z = 18, space group $R\bar{3}$] are reported in this paper.
This paper presents some of the first results of global linear stability analyses performed using a bespoke eigensolver that has recently been implemented in the next generation flow solver framework CODA. The eigensolver benefits from the automatic differentiation capability of CODA that allows computation of the exact product of the Jacobian matrix with an arbitrary complex vector. It implements the Krylov–Schur algorithm for solving the eigenvalue problem. The bespoke tool has been validated for the case of laminar flow past a circular cylinder with numerical results computed using the TAU code and those reported in the literature. It has been applied with both second-order finite volume and high-order discontinuous Galerkin schemes for the case of laminar flow past a square cylinder. It has been demonstrated that using high-order schemes on coarser grids leads to well-converged eigenmodes with a shorter computation time compared to using second-order schemes on finer grids.
In November 2018 wildfire destroyed Paradise. The town in California, that is. The so called “Camp Fire” killed 85 people in the town and surrounding area. That year also, fires burned large parts of Siberia, New Zealand and Canada, killed motorists in Portugal and Greece and eradicated crucial ecosystems in Tasmania.
These forest fires are getting hotter and bigger and are burning more places. More than ten million acres of forest burned in the United States for the first time in 2015, and then again in 2017, and in 2020. By late June in 2023, halfway through the fire season, more forest area had burned in Canada than in any previous complete season. The smoke from these wildfires in Canada caused air quality health alerts in New York and elsewhere in the United States.
In July 2023 media reports of wildfire on the island of Rhodes in the Mediterranean showed tourists struggling to escape the flames. A record-breaking hot summer in the region set the scene for wildfire. Heat records were also being broken widely elsewhere, notably in Iran and in India. In August wildfire destroyed the town of Lahaina on the island of Maui the other side of the world becoming the deadliest blaze in modern US history.
The power of these fires when they get going is staggering; temperatures get so hot that trees explode and timber-framed houses and their contents are vaporized (Vaillant 2023). Temperatures over 500°C loft smoke into the stratosphere, generating pyrocumulonimbus clouds and fire-driven weather systems. The level of destruction, of trees, houses, and whatever else gets in the way of these fires is increasing. Fighting fires requires larger and larger efforts; insurance costs for lost property are rising too.
Climate change is clearly making those wildfires worse as droughts and extreme temperatures extend fire seasons. The winter of 2019 was unusually hot and dry in Australia; its wildfires have become an ever-increasing hazard. The following year brought even more extensive wildfires and a terrible toll on wildlife and property. Dramatic pictures of people being evacuated off a beach grabbed the world's attention.
Two-dimensional compressible flows in radial equilibrium are investigated in the ideal dilute-gas regime and the non-ideal single-phase regime close to the liquid–vapour saturation curve and the critical point. Radial equilibrium flows along constant-curvature streamlines are considered. All properties are therefore independent of the tangential streamwise coordinate. A differential relation for the Mach number dependency on the radius is derived for both ideal and non-ideal conditions. For ideal flows, the differential relation is integrated analytically. Assuming a constant specific heat ratio $\gamma$, the Mach number is a monotonically decreasing function of the radius of curvature for ideal flows, with $\gamma$ being the only fluid-dependent parameter. In non-ideal conditions, the Mach number profile also depends on the total thermodynamic conditions of the fluid. For high molecular complexity fluids, such as toluene or hexamethyldisiloxane, a non-monotone Mach number profile is admissible in single-phase supersonic conditions. For Bethe–Zel'dovich–Thompson fluids, non-monotone behaviour is observed in subsonic conditions. Numerical simulations of subsonic and supersonic turning flows are carried out using the streamline curvature method and the computational fluid dynamics software SU2, respectively, both confirming the flow evolution from uniform flow conditions to the radial equilibrium profile predicted by the theory.
Using a combination of mean flow spatial linear stability and two-dimensional volume-of-fluid (VoF) simulations, the physics governing the instability of high-speed liquid sheets being injected into a quiescent gas environment is studied. It is found that the gas shear layer thickness $\delta _G$ plays an influential role, where for values $\delta _G/H\lesssim 1/8$, the growth of sinuous and varicose modes is nearly indistinguishable. Here, $H$ is the liquid sheet thickness. With larger values of $\delta _G/H$, a second peak develops in the lower wavenumber region of the dispersion relation, and becomes increasingly dominant. This second peak corresponds to a large-scale sinuous mode, and its critical wavelength $\lambda _{crit,sinuous}$ is found to scale as $\lambda _{crit,sinuous}/H = 14.26 (\delta _G/H)^{0.766}$. This scaling behaviour collapses onto a single curve for various combinations of the liquid-based Reynolds ($Re_L$) and Weber ($We_L$) numbers, provided that $\delta _G/H > O({10^{-1}})$. For the varicose modes, the shape of the dispersion relation does not change with variations in $\delta _G/H$, and the liquid shear layer thickness has an almost negligible influence on the growth of instabilities. Two-dimensional VoF simulations are employed to examine the validity of the linear stability assumptions. These simulations also show that the dominant sinuous mode remains active as the process transitions into the nonlinear regime, and that this mode is ultimately responsible for fragmenting the sheet. Based on an energy budget analysis, the most influential contributors to the growth of the sinuous mode are the gas Reynolds shear stress and the lateral working of pressure on the gas side.
Time-varying flow separation on an accelerating prolate spheroid has been studied at various angles of incidence. Instantaneous pressure and scanning stereoscopic particle image velocimetry were used to shed light on the evolution of cross-flow structures for the Reynolds number ($Re$) range of $1.0\times 10^6\leq Re \leq 1.5\times 10^6$. The movement of separation lines is examined for various model accelerations to investigate on the interplay between acceleration and flow separation. The results demonstrate that for axial accelerations, the streamwise pressure distribution in the rear part of the prolate spheroid switches from an adverse to a favourable pressure gradient. At the same time, the circumferential adverse pressure gradient present during steady motion vanishes during said accelerations. In contrast, both streamwise and circumferential adverse pressure gradients strengthen when the model is axially decelerated. These dynamic pressure distributions influence the location of the separation line, which in turn moves closer to the model meridian during accelerations while moving outwards during decelerations. The streamwise vorticity distribution and the streamwise circulation both show how the separation-line position impacts the vortex formation. A high-vorticity region near the model surface is established during acceleration. In contrast, a decelerating model leads to transport of high-vorticity fluid into the outer area of the cross-flow separation. We further assess the memory effects following the near-impulsive velocity changes. The cross-flow retains the memory of moving separation lines shortly after the acceleration. However, the separation recovers quickly to a steady state.
Inertial particles in wall-bounded turbulence are known to form streaks, but experimental evidence and predictive understanding of this phenomenon is lacking, especially in regimes relevant to atmospheric flows. We carry out wind tunnel measurements to investigate this process, characterizing the transport of microscopic particles suspended in turbulent boundary layers. The friction Reynolds number $Re_\tau = {O}(10^4)$ allows for significant scale separation and the emergence of large-scale motions, while the range of viscous Stokes number $St^+=18$–870 is relevant to the transport of dust and fine sand in the atmospheric surface layer. We perform simultaneous imaging of both carrier and dispersed phases along wall-parallel planes in the logarithmic layer, demonstrating that streamwise particle streaks largely overlap with large-scale low-speed flow regions. The fluid–particle slip velocity indicates that with increasing inertia, the particle streaks outlive the low-speed fluid streaks. Moreover, two-point statistics show that the width of the particle streaks increases linearly with Stokes number, bounded by the size of the coherent flow structures. Finally, the particle-sampled flow topology suggests that particle streaks reside between the legs of hairpin packets. From these observations, we infer a conceptual view of the formation of particle streaks in the frame of the attached eddy model. A scaling for the particle streaks’ width is derived as a function of $Re_\tau$ and $St^+$, which reproduces the measured trends and predicts widths ${O}(0.1)$ m in the atmospheric surface layer, comparable to aeolian streamers observed in the field.
We present a method for accurately determining the stability characteristics of spatially modulated shear layers. The algorithm can handle arbitrary commensurate states, which are not accessible to classical direct-numerical-simulation-based approaches. It uses spectral discretization of the field equations to handle field modulations and the spectrally accurate immersed boundary conditions method to handle the geometry modulations. The algorithm can deal with pattern interaction effects driven by modulations of different physical origins. Various tests demonstrate that the algorithm delivers spectral accuracy for eigenvalues and eigenfunctions. The algorithm can be easily extended to analyse many sources and patterns of modulation with minimal commitment to the user's time.