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Mixing and heat transfer rates are typically enhanced in high-pressure transcritical turbulent flow regimes. This is largely due to the rapid variation of thermophysical properties near the pseudo-boiling region, which can significantly amplify velocity fluctuations and promote flow destabilisation. The stability conditions are influenced by the presence of baroclinic torque, primarily driven by steep, localised density gradients across the pseudo-boiling line; an effect intensified by differentially heated wall boundaries. As a result, enstrophy levels increase compared with equivalent low-pressure systems, and flow dynamics diverge from those of classical wall-bounded turbulence. In this study the dynamic equilibrium of these instabilities is systematically analysed using linear stability theory. It is shown that under isothermal wall transcritical conditions, the nonlinear thermodynamics near the pseudo-boiling region favour destabilisation more readily than in subcritical or supercritical states; though this typically requires high-Mach-number regimes. The destabilisation is further intensified in non-isothermal wall configurations, even at low Brinkman and significantly low Mach numbers. In particular, the sensitivity of neutral curves to Brinkman number variations, along with the modal and non-modal perturbation profiles of hydrodynamic and thermodynamic modes, offer preliminary insight into the conditions driving early destabilisation. Notably, a non-isothermal set-up (where walls are held at different temperatures) is found to be a necessary condition for triggering destabilisation in low-Mach, low-Reynolds-number regimes. For the same Brinkman number, such configurations accelerate destabilisation and enhance algebraic growth compared with isothermal wall cases. As a consequence, high-pressure transcritical flows exhibit increased kinetic energy budgets, driven by elevated production rates and reduced viscous dissipation.
Biological soil crusts (biocrusts) are key components of dryland ecosystems worldwide, contributing to soil stabilization, nutrient cycling and enhancing ecosystem resilience. Despite their ecological importance, biocrusts in the Arabian Peninsula are largely underexplored, with much of the region’s biocrust diversity and functionality remaining undocumented. This review synthesizes current knowledge on biocrusts across the Arabian Peninsula, focusing on their major taxonomic groups (cyanobacteria, fungi, lichens, mosses and algae), their ecological roles and distribution patterns. It also discusses the potential for biocrust restoration through strategies such as cyanobacterial inoculation and passive protection, which could contribute to land degradation and desertification control in the Arabian Peninsula. Our work identifies significant research gaps in biocrust biodiversity, ecophysiology and their role in ecosystem functioning within this region, and calls for more focused research to integrate biocrusts into land management strategies for the Arabian Peninsula.
This study traces the evolution and the fate of two Icelandic glaciers, Hofsjökull eystri in the southeast and Okjökull in the west, from their Little Ice Age maximum (∼1890) to the present. Glacier maximum extents were reconstructed using historical maps, written descriptions, geomorphological evidence, and aerial and satellite imagery. Time series of digital elevation models and a 2025 radio echo sounding survey provide further insight into changes in surface area, volume and bedrock topography. Despite similar latitudes (∼64.4°N) and elevation ranges (∼900–1150 m a.s.l.), the glaciers reside in different climate regimes. Both glaciers covered ∼7 km2 in the 1940s. Since then, Okjökull has been declared vanished and Hofsjökull eystri has lost ∼70% of its area and ∼90% of its volume, with a maximum thickness of 55 m in 2024. Projections suggest that, at the current rate of thinning, Hofsjökull eystri will disappear entirely within the next 30–45 years.
The Boltzmann kinetic equation is considered to compute the transport coefficients associated with the mass flux of intruders in a granular gas. Intruders and granular gas are immersed in a gas of elastic hard spheres (molecular gas). We assume that the granular particles are sufficiently rarefied so that the state of the molecular gas is not affected by the presence of the granular gas. Thus, the gas of elastic hard spheres can be considered as a thermostat (or bath) at a fixed temperature $T_g$. In the absence of spatial gradients, the system achieves a steady state where the temperature of the granular gas $T$ differs from that of the intruders $T_0$ (energy non-equipartition). Approximate theoretical predictions for the temperature ratio $T_0/T_g$ and the kurtosis $c_0$ associated with the intruders compare very well with Monte Carlo simulations for conditions of practical interest. For states close to the steady homogeneous state, the Boltzmann equation for the intruders is solved by means of the Chapman–Enskog method to first order in the spatial gradients. As expected, the diffusion transport coefficients are given in terms of the solutions of a set of coupled linear integral equations which are approximately solved by considering the first Sonine approximation. In dimensionless form, the transport coefficients are nonlinear functions of the mass and diameter ratios, the coefficients of restitution and the (reduced) bath temperature. Interestingly, previous results derived from a suspension model based on an effective fluid–solid interaction force are recovered when $m/m_g\to \infty$ and $m_0/m_g\to \infty$, where $m$, $m_0$ and $m_g$ are the masses of the granular particles, intruders and molecular gas particles, respectively. Finally, as an application of our results, thermal diffusion segregation is exhaustively analysed.
Linear-stability modelling suggests that all sufficiently large riblets promote maximally growing spanwise rollers (García-Mayoral & Jiménez 2011 J. Fluid Mech. vol. 678, 317–347), yet direct numerical simulations (DNS) have shown that this is not the case (Endrikat et al. 2021 J. Fluid Mech. vol. 913, A37) some riblet shapes do not form spanwise rollers at all. Thus, the drag-reduction breakdown across all riblet shapes cannot be solely attributed to maximally growing spanwise rollers, prompting a reappraisal of the modelling. In this paper, comparing DNS data with riblet-resolving linear-stability predictions shows that the spanwise rollers are actually marginal modes, not maximally growing instabilities. This riblet-resolved linear analysis also predicts that not all riblet shapes promote spanwise rollers, in agreement with DNS, and unlike earlier linear-stability modelling, which relied on a one-dimensional (1-D) mean flow and on an over-simplified effective wall-admittance boundary condition. These riblet-resolved calculations further inform how to capture the effect of the riblet shape in a 1D model. Once captured, predictions with an effective boundary condition match riblet-resolved results, but still do not indicate what features of the riblet geometry promote the roller instability. Thus, the wall admittance is measured near the riblet crests, in both the riblet-resolved linear analysis and DNS, to show that the in-groove dynamics is dominated by a balance between the overlying pressure and unsteady inertia, and not viscous diffusion, as previously assumed. This pressure–unsteady-inertia balance sets the linear scaling of the wall admittance with riblet size, as observed in DNS, and is a key factor in setting the streamwise wavelength of the spanwise rollers. Furthermore, modelling this pressure–unsteady-inertia balance in the wall admittance reveals the role of riblet slenderness in promoting spanwise rollers, which provides the missing link in previous correlations between the riblet geometry and the presence or lack of rollers.
We investigate Lighthill’s proposed turbulent mechanism for near-wall concentration of spanwise vorticity by calculating mean flows conditioned on motion away from or toward the wall in an (friction Reynolds number) ${\textit{Re}}_\tau =1000$ database of plane-parallel channel flow. Our results corroborate Lighthill’s proposal throughout the entire logarithmic layer, but extended by counter-flows that help explain anti-correlation of vorticity transport by advection and by stretching/tilting. We present evidence also for Lighthill’s hypothesis that the vorticity transport in the log layer is a ‘cascade process’ through a scale hierarchy of eddies, with intense competition between transport outward from and inward to the wall. Townsend’s model of attached eddies of hairpin-vortex type accounts for half of the vorticity cascade, whereas we identify necklace type or ’shawl vortices’ that envelop turbulent sweeps as supplying the other half.
Kant and Environmental Philosophy starts with problems of the Anthropocene and looks to Immanuel Kant for answers. It offers a close reading of Kant's texts, arguing that the views we find in his ethical, political, and aesthetic theory are helpful for making sense of ecological challenges like climate change. The book clarifies our duties regarding climate extinction, geoengineering, consumerism, and future generations. It provides insights and solutions for obstacles to sustainability, including corruption and the possibility of civil collapse. In environmental philosophy, historical commentators mine familiar philosophers for insights to these problems, but Kant is often seen as an anthropocentric and dualistic individualist in a world dominated by consequentialist thinking, and accordingly he is overlooked as relevant for environmental philosophy. This book challenges that conclusion, and its comprehensive examination of Kant's texts provides lessons for environmental philosophy and climate ethics at a time when a fresh perspective is desperately needed.
States of Transition takes a deep dive into the multiple roles states are playing in supporting transitions to a more sustainable world and where there is scope for their transformation. Going beyond unhelpful binaries - which cast the state as the central problem or the all-encompassing solution to ecological and social crises - it explores diverse current state practice across key domains: military, democracy, welfare, entrepreneurial, industrial, and foreign policy. It builds on theoretical resources from a range of disciplines, as befits the challenge of making sense of these diverse aspects of state power. It moves beyond existing analysis of the 'environmental state' to explore scope for a 'transition state' to emerge, capable of corralling and transforming all aspects of state power behind the goal of responding to the existential threat of planetary collapse. The book will be invaluable to students, academics, and practitioners concerned with environmental policy and sustainability.
This chapter explores the evolving legal and regulatory landscape within the Gulf states, focusing on Qatar, Saudi Arabia, and the UAE, as these countries strive to curtail carbon emissions. This chapter also offers a prescriptive analysis, proposing custom-designed legal and regulatory frameworks specifically tailored to the unique economic and legal environments of each nation. This analysis details viable carbon reduction strategies that not only promote environmental sustainability and meet their climate pledges but also bolster economic growth, fostering a win–win scenario for the Gulf states. This chapter presents a strategic roadmap for implementing these initiatives within each country’s specific macroeconomic context. By offering actionable and contextually relevant strategies for impactful climate action, this chapter aims to significantly enrich the dialogue on environmental policy and climate change mitigation efforts in the Gulf region.
This chapter narrates the historical context that shaped the contemporary economic landscape of the Gulf states and critically examines the enduring impact of colonialism on the region’s economic fabric and how the entrenched “dual economic framework” imposed limitations on development. This chapter also sheds light on the emergence of resource nationalism as a transformative strategy for Gulf states to assert control over their natural resources and challenge this dependency. The creation of OPEC serves as a core moment in the realm of global energy politics, symbolizing a strategic move towards economic autonomy and the collective bargaining power of developing countries. Building upon this historical foundation, the chapter deconstructs the philosophical and theoretical frameworks that underpin development strategies during this era of rapid modernization in the Gulf and explores how Gulf policymakers creatively adapted these models to their unique socio-political and economic contexts, paving the way for their ascent as significant players in the global energy market.
Despite five decades of analysis, many aspects of Mars crater morphology and evolution remain enigmatic, and it seems likely that new types of data will be needed to find the answers. As a final section in this chapter, we offer new approaches to solving these questions. Finding the answers will require a new orbital data set. Our recommendation is for a new data set that is comparable to many that have been collected for other planets in the Solar System and thus well within the capabilities of the National Air and Space Administration (NASA) and other international space agencies.
We take the younger examples, as illustrated in Chapter 4, and show some of the common ways that craters may be modified. Even craters that are classified as morphologically fresh may have experienced modification. This might take the form of chemical weathering of the floor or deposition of eolian or ice deposits within the crater cavity.
This chapter reviews impact craters throughout the Solar System, looking first at craters formed on Earth, where we have the best field knowledge. We then investigate craters formed on airless rocky bodies (the Moon and Mercury), where the cratering process is not affected by atmospheric effects. We follow this with a glimpse of craters on volatile-rich bodies that also lack an atmosphere, specifically Ganymede, 1 Ceres, and Charon. Here the target material is most likely water ice. Finally, we examine craters formed on bodies with thick atmospheres (Venus and Titan) to see what landforms may have been formed by the interaction of the projectile and the ejecta with the atmosphere.