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The meteorology of the stratosphere in the Southern Hemisphere (SH) plays a critical role in the variability of the ozone hole and also has a major influence on surface climate and weather. The predominant feature of the stratosphere is a band of strong mid- to high-latitude westerlies that surround a very cold pole and exist from autumn to spring. This ‘polar vortex’ is stronger and less variable in the SH than in the Northern Hemisphere, and the low temperatures and isolation within the vortex are key conditions necessary for rapid chemical destruction of Antarctic ozone. The largest interannual variability in the SH occurs in spring and is associated primarily with variability in the strength and timing of the seasonal breakdown of the polar vortex. Interannual variability and trends in the timing of the vortex breakdown are coupled to variability and trends in the summertime Southern Annular Mode and its associated influence on tropospheric and surface climate. A rapid warming of the polar stratosphere and weakening of the westerlies occurred in September 2002 and 2019, resulting in small ozone holes for those years. These are the only two observed occurrences of such events in the SH. In addition, observations show significant trends in vortex characteristics (colder, stronger winds, later breakup) during the 1980s and 1990s, but not since 2000. These pre-2000 trends and post-2000 pause are consistent with Antarctic ozone hole trends (growth, followed by initial signs of recovery) since the 1980s. Interactions between ozone chemistry and the stratospheric circulation, which occurs across timescales, can enhance the coupling of the stratosphere to the troposphere, with implications for both interannual and long-term changes in SH weather and climate.
This chapter reviews the recent literature on the meteorology and climate of the African region in the Southern Hemisphere focusing on key features of circulation and its seasonal shifts, including the rain-bearing weather systems. It is only in the very recent literature that several very important regional circulation features have been documented in detail. These advances have been aided by more accurate reanalyses, high-resolution satellite observations, and models, augmenting vast areas of sparse surface and upper-air observations in the African region. The chapter highlights prominent synoptic and mesoscale circulation features such as the Mozambique Channel Trough, the Botswana High, the Angola Low, the Congo Air Boundary, low-level jets, atmospheric rivers, and ridging South Atlantic anticyclones. It details the dynamics and variability of rainfall-bearing synoptic-scale systems such as cut-off low-pressure systems, tropical–extratropical cloud bands, and the role of Rossby wave propagation and breaking associated with these systems. The chapter also deals with key ocean circulation features such as the Angola-Benguela Frontal Zone, the Seychelles-Chagos Thermocline Ridge, the Agulhas Current retroflection and leakage into the South Atlantic, eddies and meanders on this current and in the Mozambique Channel, as well as sea-surface temperature variability in the neighbouring oceans such as the Benguela Niño and dipoles in the Indian Ocean. In addition, the chapter covers climate variability in the region on a variety of timescales from the intraseasonal to interannual and trends at longer timescales. The latter part focuses on advances in applications of numerical weather models and ensemble prediction systems, seasonal climate forecasting, and climate change projections. In conclusion, the chapter provides an analysis of current limitations and offers recommendations for future research.
This chapter provides a comprehensive overview of stratosphere–troposphere interactions, with emphasis on the Southern Hemisphere. We introduce key concepts such as wave activity (Eliassen–Palm fluxes), the Charney–Drazin criterion for wave propagation, downward control, and radiative coupling. The chapter then explores the stratosphere’s influence on tropospheric timescales and the surface impacts of dynamical perturbations originating in the stratosphere. It delves into subseasonal to seasonal prediction, highlighting the enhanced forecasting skill derived from stratospheric dynamics. The discussion also addresses the impact of stationary waves and model biases on stratosphere–troposphere coupling. Furthermore, the chapter examines the stratosphere’s role in shaping tropospheric circulation over longer timescales, including the effects of climate change and the potential influence of the ozone hole. Finally, it investigates the interactions between the Quasi-Biennial Oscillation and the Madden–Julian Oscillation, providing a holistic view of the complex interplay between these atmospheric layers.
A thin, evaporating sessile droplet with a pinned contact line containing inert particles is considered. In the limit in which the liquid flow decouples from the particle transport, we discuss the interplay between particle advection, diffusion and adsorption onto the solid substrate on which the droplet sits. We perform an asymptotic analysis in the physically relevant regime in which the Péclet number is large, i.e. ${\textit{Pe}}\gg 1$, so that advection dominates diffusion in the droplet except in a boundary layer near the contact line, and in which the ratio of the particle velocities due to substrate adsorption and diffusion is at most of order unity as ${\textit{Pe}}\rightarrow \infty$. We use the asymptotic model alongside numerical simulations to demonstrate that substrate adsorption leads to a different leading-order distribution of particle mass compared with cases with negligible substrate adsorption, with a significant reduction of the mass in the suspension – the nascent coffee ring reported in Moore et al. (J. Fluid Mech., vol. 920, 2021, A54). The redistribution leads to an extension of the validity of the dilute suspension assumption, albeit at the cost of breakdown due to the growth of the deposited layer, which are important considerations for future models that seek to accurately model the porous deposit regions.
Ionic surfactants are commonly employed to modify the rheological properties of fluids, particularly in terms of surface viscoelasticity. Concurrently, external electric fields can significantly impact the dynamics of liquid threads. A key question is how ionic surfactants affect the dynamic behaviour of threads in the presence of an electric field? To investigate this, a one-dimensional model of a liquid thread coated with surfactants within a radial electric field is established, employing the long-wave approximation. We systematically investigate the effects of dimensionless parameters associated with the surfactants, including surfactant concentration, dilatational Boussinesq number ${\textit{Bo}}_{\kappa \infty }$ and shear Boussinesq number ${\textit{Bo}}_{\mu \infty }$. The results indicate that increasing the surfactant concentration and the two Boussinesq numbers reduces both the maximum growth rate and the dominant wavenumber. In addition, both the electric field and surfactants mitigate the breakup of the liquid thread and the formation of satellite droplets. At low applied electric potentials, the surface viscosity induced by surfactants predominantly governs this suppression. Surface viscosity suppresses the formation of satellite droplets by maintaining the neck point at the centre of the liquid thread within a single disturbance wavelength. When the applied potential is high, the electric stress has two main effects: the external electric field exerts a normal pressure on the liquid thread surface, suppressing satellite droplet formation, while the internal electric field inhibits liquid drainage. Surface viscosity further stabilizes the system by suppressing flow dynamics during this process.
Sustainable management of watersheds to secure freshwater resources and maintain ecological stability relies on adopting land-use strategies supporting diverse ecosystem services through natural processes. This necessitates systematic evaluation of prospective land-use practices and their associated costs and benefits. We conducted a comprehensive economic evaluation of pro-watershed land-use options, focusing on a well-recognized agroforestry system with alternative organic cultivation in the Navnera watershed in Rajasthan, India. We adopted the ‘total economic valuation’ framework, using the revealed preference approach for monetary evaluation and modelling indirect benefits primarily through Integrated Valuation of Ecosystem Services and Tradeoffs (InVEST). Our findings indicate that the total economic value of ecosystem services in this watershed has the potential to increase by 4.6% with the adoption of agroforestry and only by 1.3% under organic farming compared to current land-use practices. While agroforestry might reduce farmland revenue and water yield, it compensates for these with other important environmental benefits such as water purification, sediment reduction, nutrient retention and carbon sequestration. This local-scale appraisal of ecosystem services helps policymakers understand the cost–benefit dynamics of watershed land-use changes, which is vital for developing effective management strategies through the involvement of local communities.
As a step towards realising a skin-friction drag reduction technique that scales favourably with Reynolds number, the impact of a synthetic jet on a turbulent boundary layer was explored through a study combining wind-tunnel measurements and large eddy simulations. The jet was ejected in the wall-normal direction through a rectangular slot whose spanwise dimension matched that of dominant large-scale structures in the logarithmic region to target structures of that size and smaller simultaneously. Local skin-friction reduction was observed at both $x/\delta =2$ and $x/\delta =5$ downstream of the orifice centreline, where $\delta$ is the boundary-layer thickness. At $x/\delta =2$, the skin-friction reduction was observed to be due to the synthetic-jet velocity deficit intersecting the wall. At $x/\delta =5$, evidence from the simulations and wind-tunnel measurements suggests that a weakening of wall-coherent velocity scales is primarily responsible for the skin-friction reduction. Local skin-friction reduction which scales favourably with Reynolds number may be achievable with the synthetic jet employed in this study. However, there are many technical hurdles to overcome to achieve net skin-friction drag reduction over the entire region of influence. For instance, regions of skin-friction increase were observed close to the orifice ($x/\delta \lt 2$) and downstream of the orifice edge due to the induced motion of synthetic-jet vortical structures. Additionally, a recirculation region was seen to form during expulsion, which has implications for pressure drag on non-planar surfaces.
Northern Calabria forms part of the Calabrian Arc, a geologically complex region in southern Italy shaped by the convergence between the Eurasian and African plates. This convergence drove the closure of the Tethys Ocean and produced the subsequent phases of collisional and extensional tectonics. Thrusting during the Alpine orogeny produced extensive nappe stacking, followed by structural reorganization and exhumation during the Oligocene-Miocene. Tectonostratigraphically, the Apennine carbonate platform forms the lowest structural unit, overlain successively by the Liguride Oceanic Complex and the Calabride Complex, which includes the Sila nappe stack. Along Calabria’s eastern Ionian margin, forearc basins developed in response to the retreating subduction zone. To better constrain sediment routing pathways and regional uplift in northern Calabria from early to late Miocene, a multi-proxy provenance study was applied to four forearc basins: Rossano, Cirò, Crotone and Catanzaro. Quantitative heavy-mineral analysis, single-grain garnet and apatite chemistry, and apatite U–Pb chronology reveal spatial and temporal variations in sediment sources. Siliciclastic samples, spanning Aquitanian to Messinian in age, record changing contributions from a combination of low- to high-grade metamorphic and plutonic sources, including mafic Liguride units. Up-section shifts in sediment sourcing patterns indicate that Calabrian Arc exhumation and uplift, characterized by a rapid increase in the middle Miocene followed by a slow reduction in relief, played a pivotal role in controlling the timing and direction of sediment transport. This study demonstrates the benefits of multi-method provenance approaches to achieve valuable insights into relief build-up and demise, associated divide migration and sedimentary responses within a young and complex, zircon-poor orogenic arc system.
This chapter offers an overview of Antarctica’s major meteorological and climate features using the latest methods, data products, and research findings. The first half of the chapter presents a thorough description of the Antarctic geography and its climatological temperature, precipitation, and near-surface environment. It provides a dedicated section covering Antarctic foehn and foehn-induced warming, which have been identified as major ‘hot spots’ for Antarctic surface melt and ice shelf destabilisation. Next the chapter details the major large-scale and regional atmospheric circulation patterns that characterise the high southern latitudes and strongly influence Antarctic meteorology, including the Southern Annular Mode, teleconnections associated with the El Niño Southern Oscillation, and the Amundsen Sea Low. We then present the latest research discoveries on Antarctic climate extremes, with a focus on Antarctic ‘atmospheric rivers’ and their role in driving extreme temperature, precipitation, and surface melt events. The chapter closes with a summary of recent Antarctic climate change, current research gaps and challenges, and recommendations for future work.
The oceans play a fundamental role in shaping the Southern Hemisphere climate, including aspects such as why the western tropical Pacific is warmer and rainier than the eastern Pacific or why some regions in Africa, Australia, and South America often experience intense drought, heatwaves, and extreme rainfall. Eighty percent of the Southern Hemisphere is covered by oceans, encompassing the Pacific, Indian, Atlantic, and Southern Oceans in which oceanic circulations, and their interplay with the atmosphere, give rise to some of the Earth’s most powerful climate phenomena that impact regions across the Southern Hemisphere. Climate processes across these ocean sectors interact with one another through the oceans and atmosphere, adding a layer of complexity in understanding climate phenomena and in robust future projections. The oceans play a vital role in regulating the climate as the planet warms under increasing greenhouse forcing.
The triadic interactions and nonlinear energy transfer are investigated in a subsonic turbulent jet at $Re = 450\,000$. The primary focus is on the role of these interactions in the formation and attenuation of streaky structures. To this end, we employ bispectral mode decomposition, a technique that extracts coherent structures associated with dominant triadic interactions. A strong triadic correlation is identified between Kelvin–Helmholtz (KH) wavepackets and streaks: interactions between counter-rotating KH waves generates streamwise vortices, which subsequently give rise to streaks through the lift-up mechanism. The most energetic streaks occur at azimuthal wavenumber $m = 2$, with the dominant contributing triad being $[m_1, m_2, m_3] = [1, 1, 2]$. The spectral energy budget reveals that the net effect of nonlinear triadic interactions is an energy loss from the streaks. As these streaks convect downstream, they engage in further nonlinear interactions with other frequencies, which drain their energy and ultimately lead to their attenuation. Further analysis identifies the dominant scales and direction of energy transfer across different spatial regions of the jet. While the turbulent jet exhibits a forward energy cascade in a global sense, the direction of energy transfer varies locally: in the shear layer near the nozzle exit, triadic interactions among smaller scales dominate, resulting in an inverse energy cascade, whereas farther downstream, beyond the end of the potential core, interactions among larger scales prevail, leading to a forward cascade.
Secondary flows induced by spanwise heterogeneous surface roughness play a crucial role in determining engineering-relevant metrics such as surface drag, convective heat transfer and the transport of airborne scalars. While much of the existing literature has focused on idealized configurations with regularly spaced roughness elements, real-world surfaces often feature irregularities, clustering and topographic complexity for which the secondary flow response remains poorly understood. Motivated by this gap, we investigate multicolumn roughness configurations that serve as a regularized analogue of roughness clustering. Using large-eddy simulations, we systematically examine secondary flows across a controlled set of configurations in which cluster density and local arrangement are varied in an idealized manner, and observe that these variations give rise to distinct secondary flow polarities. Through a focused parameter study, we identify the spanwise gap between the edge-most roughness elements of adjacent columns, normalized by the channel half-height ($s_a/H$), as a key geometric factor governing this polarity. In addition to analysing the time-averaged structure, we investigate how variations in polarity affect the instantaneous dynamics of secondary flows. Here, we find that the regions of high- and low-momentum fluid created by the secondary flows alternate in a chaotic, non-periodic manner over time. Further analysis of the vertical velocity signal shows that variability in vertical momentum transport is a persistent and intrinsic feature of secondary flow dynamics. Taken together, these findings provide a comprehensive picture of how the geometric arrangement of roughness elements governs both the mean structure and temporal behaviour of secondary flows.
A fully resolved numerical study was performed to investigate interfacial heat and mass transfer enhanced by the fully developed Rayleigh–Bénard–Marangoni instability in a relatively deep domain. The instability was triggered by evaporative cooling modelled by a constant surface heat flux. The latter allowed for temperature-induced variations in surface tension giving rise to Marangoni forces reinforcing the Rayleigh instability. Simulations were performed at a fixed Rayleigh number (${\textit{Ra}}_h$) and a variety of Marangoni numbers (${\textit{Ma}}_h$). In each simulation, scalar transport equations for heat and mass concentration at various Schmidt numbers (${\textit{Sc}}=16{-}200$) were solved simultaneously. Due to the fixed (warm) temperature prescribed at the bottom of the computational domain, large buoyant plumes emerged quasi-periodically both at the top and bottom. With increasing Marangoni number a decrease in the average convection cell size at the surface was observed, with a simultaneous improvement in near-surface mixing. The presence of high aspect ratio rectangular convection cell footprints was found to be characteristic for Marangoni-dominated flows. Due to the promotion of interfacial mass transfer by Marangoni forces, the power in the scaling of the mass transfer velocity, $K_{\!L}\!\propto\! \textit{Sc}^{-n}$, was found to decrease from $n=0.50$ at ${\textit{Ma}}_h=0$ to $\approx 0.438$ at ${\textit{Ma}}_h=13.21\times 10^5$. Finally, the existence of a buoyancy-dominated and a Marangoni-dominated regime was investigated in the context of the interfacial heat and mass transfer scaling as a function of ${\textit{Ma}}_h+\varepsilon {\textit{Ra}}_h$, where $\varepsilon$ is a small number determined empirically.