To save content items to your account,
please confirm that you agree to abide by our usage policies.
If this is the first time you use this feature, you will be asked to authorise Cambridge Core to connect with your account.
Find out more about saving content to .
To save content items to your Kindle, first ensure no-reply@cambridge.org
is added to your Approved Personal Document E-mail List under your Personal Document Settings
on the Manage Your Content and Devices page of your Amazon account. Then enter the ‘name’ part
of your Kindle email address below.
Find out more about saving to your Kindle.
Note you can select to save to either the @free.kindle.com or @kindle.com variations.
‘@free.kindle.com’ emails are free but can only be saved to your device when it is connected to wi-fi.
‘@kindle.com’ emails can be delivered even when you are not connected to wi-fi, but note that service fees apply.
A model for galloping detonations is conceived as a sequence of very fast re-ignitions followed by long periods of evolution with quenched reactions. Numerical simulations of the one-dimensional Euler equations are conducted in this limit. While the mean speed and structure is found in reasonable agreement with Chapman–Jouguet theory, very strong pulsations of the lead shock appear, along with a train of rear-facing N-waves. These dynamics are analysed using characteristics. A closed-form solution for the lead shock dynamics is formulated, which is found in excellent agreement with numerics. The model relies on the presence of a single time scale of the process, the pulsation period, which controls the shock dynamics via the shock change equations and establishes a shock decay with a single time constant. These long periods of shock decay with known dynamics are punctuated by energy release events, with ‘kicks’ in the shocked speed controlled by the pressure increase and resulting lead shock amplification. Model predictions are found in excellent agreement with previous numerical results of pulsating detonations far from the stability limit.
Paleontology provides insights into the history of the planet, from the origins of life billions of years ago to the biotic changes of the Recent. The scope of paleontological research is as vast as it is varied, and the field is constantly evolving. In an effort to identify “Big Questions” in paleontology, experts from around the world came together to build a list of priority questions the field can address in the years ahead. The 89 questions presented herein (grouped within 11 themes) represent contributions from nearly 200 international scientists. These questions touch on common themes including biodiversity drivers and patterns, integrating data types across spatiotemporal scales, applying paleontological data to contemporary biodiversity and climate issues, and effectively utilizing innovative methods and technology for new paleontological insights. In addition to these theoretical questions, discussions touch upon structural concerns within the field, advocating for an increased valuation of specimen-based research, protection of natural heritage sites, and the importance of collections infrastructure, along with a stronger emphasis on human diversity, equity, and inclusion. These questions offer a starting point—an initial nucleus of consensus that paleontologists can expand on—for engaging in discussions, securing funding, advocating for museums, and fostering continued growth in shared research directions.
This numerical investigation focuses on the mechanisms, flow topology and onset of Kelvin–Helmholtz instabilities (KHIs), that drive the leading-edge shear-layer destabilisation in the wake of wall-mounted long prisms. Large-eddy simulations are performed at ${\textit{Re}} = 2.5\times 10^3, 5\times 10^3$ and $1\times 10^4$ for prisms with a range of aspect ratio (AR, height-to-width) between $0.25$ and $1.5$, and depth ratios (DR, length-to-width) of $1{-}4$. Results show that shear-layer instabilities enhance flow irregularity and modulate spanwise vortex structures. The onset of KHI is strongly influenced by depth ratio, such that long prisms (${\textit{DR}}= 4$) experience earlier initiation compared with shorter ones (${\textit{DR}}= 1$). At higher Reynolds numbers, the onset of KHI shifts upstream towards the leading-edge, intensifying turbulence kinetic energy and increasing flow irregularity, especially for long prisms. The results further show that in this configuration, energy transfer from the secondary recirculation region contributes to the destabilisation of the leading-edge shear layer by reinforcing low-frequency modes. A feedback mechanism is identified wherein energetic flow structures propagate upstream through reverse boundary-layer flow, re-energising the leading-edge shear layer. Quantification using probability density functions reveals rare, intense upstream energy convection events, driven by this feedback mechanism. These facilitate the destabilisation process regardless of Reynolds number. This study provides a comprehensive understanding of the destabilisation mechanisms for leading-edge shear layers in the wake of wall-mounted long prisms.
Large-scale circulation involves the interaction of the lower and middle-upper troposphere, influencing synoptic-scale circulation, regional climate, teleconnections, and paleoclimate proxies. Described by the westerly vortex and jetstreams, the subtropical ridge, vortex asymmetry, and the South Pacific Split Jet, it is a framework for interpreting the natural archive and proxies. Southern and Northern Hemisphere pressure fields are described through planetary wave modes and zonal wave number indices. Anticyclone, cyclone, subtropical, mid-latitude, and subpolar storm-track and blocking climatologies and their influence on climate and hydrological change are presented. The chapter covers synoptic circulation, classical air-mass types, their source regions and temperature/humidity characteristics, and air-mass streamline trajectories; tropical depressions and cyclone storm tracks, easterly waves, blocking, and subtropical cyclones; mid-latitude synoptic systems including frontal lows, cut-off lows, and cold air outbreaks; and tropical–extratropical interaction with cloud bands, tropical–temperate troughs, atmospheric rivers, and warm-air incursions to the poles.
Undulatory slender objects have been a central theme in the hydrodynamics of swimming at low Reynolds number, where the slender body is usually assumed to be inextensible, although some microorganisms and artificial microrobots largely deform with compression and extension. Here, we theoretically study the coupling between the bending and compression/extension shape modes, using a geometrical formulation of kinematic microswimmer hydrodynamics to deal with the non-commutative effects between translation and rotation. By means of a coarse-grained minimal model and systematic perturbation expansions for small bending and compression/extension, we analytically derive the swimming velocities and report three main findings. First, we revisit the role of anisotropy in the drag ratio of the resistive force theory, and generally demonstrate that no motion is possible for uniform compression with isotropic drag. We then find that the bending–compression/extension coupling generates lateral and rotational motion, which enhances the swimmer’s manoeuvrability, as well as changes in progressive velocity at a higher order of expansion, while the coupling effects depend on the phase difference between the two modes. Finally, we demonstrate the importance of often-overlooked Lie bracket contributions in computing net locomotion from a deformation gait. Our study sheds light on compression as a forgotten degree of freedom in swimmer locomotion, with important implications for microswimmer hydrodynamics, including understanding of biological locomotion mechanisms and design of microrobots.
This chapter covers methods used to extract and interpret paleoclimate time series of climate modes, surface ocean, hydroclimate, and sea-level variability. The coral reef environment is explored as an archive of sea-surface temperature and salinity, hydroclimate, tradewinds, cloud cover and ocean circulation, storms, and regional and global sea-level variability, using stable isotopes, trace element analysis, radioisotopes, ultraviolet, and x-ray stratigraphic methods. The comparative tropical terrestrial hydroclimate record is investigated through the tree-ring and speleothem archive using traditional (dendrochronology and stable isotopes) and emerging methods such as biomarkers. Tropical hydroclimate reconstructions are presented, with the current understanding of decadal-scale variability due to the PDO/IPO. The coral and bivalve shell archive is presented as a record of boundary current, variability of continental shelf wind and current, and marine heat waves. Case studies reconstruct coastal jet modes and marine heat wave events for the Peruvian Current, Peru–Chile, and the Ningaloo Current, western Australia, in conjunction with ENSO variability during the Holocene.
Weather regime type and frequency are key diagnostics to interpret regional climate. The statistical methods used to downscale the centres of action in the mean atmospheric state to their family of weather regimes (WR) according to climate mode phases are presented in detail. The North Atlantic–European region is used as an example of WR decomposition of the mean climate. The chapter focuses on the identification of WR types for each region of the Southern Hemisphere and their spatio-temporal variability in relation to climate mode phase. These are the reference WRs for the interpretation of synoptic paleoclimate in each of the climate proxy chapters that follow. WRs are presented for the Maritime Continent, northern and central Australia, South Pacific Convergence Zone, Tasman Sea, New Zealand and southwest Pacific, eastern Pacific, Brazil to Uruguay, southwest Africa, southern Africa, eastern Africa, subtropical western Australia, southwestern Australia, southeastern Australia, the south Indian, south Pacific, and south Atlantic sectors of the Southern Ocean, and coastal Antarctica, including Patagonian South America, the Antarctic Peninsula, and the East Antarctic.
The unique reproductive strategies of botryllid ascidians, which include both asexual and sexual mechanisms as well as an extensive capacity for regeneration, contribute to their fast population growth and wide-ranging ecological effects. These colonial organisms have unique ecological adaptations and responses to environmental factors, yet comprehensive comparative studies on their environmental preferences remain scarce. We conducted an experimental study to explore the asexual reproduction and regeneration response of Botrylloides niger and Botryllus humilis colonies to varying salinity (36.5–39.5 PSU) and temperature (26 ± 1–30 ± 1°C) levels. Experimental findings highlighted species-specific preferences and stress responses: B. niger demonstrated higher tolerance to elevated salinity (39.5 PSU) with optimal growth rates at 26 ± 1–30 ± 1°C, whereas B. humilis displayed a preference for lower salinity and tendencies towards vascular budding at higher temperatures (30 ± 1°C). These observations suggest potential niche differentiation and ecological success, particularly in Mediterranean conditions, implying possible coexistence without intense competition in similar habitats. This research offers insights into the adaptive mechanisms of these ascidians, shedding light on their ecological roles and potential implications in coastal ecosystems amid changing environmental scenarios.
This chapter focuses on the glaciochemistry of Antarctic ice cores and their applications as aerosol tracers of atmospheric, sea ice, and oceanic variability. Marine aerosol–climate relationships are discussed using marine boundary layer, air–sea exchange, and cloud science. Glaciochemistry theory is presented for interpreting marine ion concentrations in ice cores as circumAntarctic wind-field and paleoweather tracers, sea ice extent, concentration, and polynya tracers. Similarly, non-marine aerosol ion glaciochemistry is examined, with applications including nitrate concentration as polar stratosphere and katabatic wind-field proxies; non-sea-salt sulphate as a volcanism proxy; and mineral dust as long-range air-mass tracers. Dust typing and mineral fingerprinting methods are discussed to identify Southern Hemisphere source areas. Air mass trajectory methods, both forward and backward, are presented to relate ice core ion glaciochemistry and dust particles as aerosol tracers to reconstruct large-scale atmospheric circulation, climate mode, and regional weather regime history during the interglacial and glacial periods.
This chapter covers the response of tropical to subantarctic glaciers to variability in tropospheric and sea-surface temperature, lapse rates, and precipitation. Glacial behaviour is reflected in regional weather patterns: air mass transport, temperature, precipitation and humidity, insolation/cloud cover, wind speed, and large-scale circulation. Glacier types, climate zones, and physical processes are used to define the latitudinal continuum of climate–glacier coupling. The glacial archive is examined using indicators of glacial structure and geomorphology, their mapping, and geochronological methods. Glacier mass balance characteristics are defined by climate and glacier morphometrics, including equilibrium line altitude, vertical balance profiles, glacier tongue length, balance ratios, and accumulation–area, area–altitude, and geomorphic–altitude relationships. Glacier mass balance and reaction times are examined via energy balance, glacier dynamics, and flow-line modelling. Approaches to reconstructing glacial behaviour include numerical weather forecast modelling and synoptic typing based on ice core geochemistry and relationships to weather regimes and climate variability.
We study the dynamics of salt fingers in the regime of slow salinity diffusion (small inverse Lewis number) and strong stratification (large density ratio), focusing on regimes relevant to Earth’s oceans. Using three-dimensional direct numerical simulations in periodic domains, we show that salt fingers exhibit rich, multiscale dynamics in this regime, with vertically elongated fingers that are twisted into helical shapes at large scales by mean flows and disrupted at small scales by isotropic eddies. We use a multiscale asymptotic analysis to motivate a reduced set of partial differential equations that filters internal gravity waves and removes inertia from all parts of the momentum equation except for the Reynolds stress that drives the helical mean flow. When simulated numerically, the reduced equations capture the same dynamics and fluxes as the full equations in the appropriate regime. The reduced equations enforce zero helicity in all fluctuations about the mean flow, implying that the symmetry-breaking helical flow is generated spontaneously by strictly non-helical fluctuations.
Synoptic paleoclimatology is an interdisciplinary approach, using atmospheric, oceanic, and earth sciences to connect paleoweather and paleoclimate. The weather regime approach to paleoclimatology identifies large-scale flow patterns in the atmosphere and ocean, their persistence or transience, and associated weather characteristics. Weather-event frequency is expressed in the paleoclimate signal. Paleoweather is explored within scaling climate modes of variability: latitudinal insolation and temperature gradients associated with orbital forcing, and internal dynamical modes of variability in the atmosphere and ocean. The chapter covers the modern global atmospheric pressure field and its geographic centres of action; the role of wind and wind stress on ocean circulation; ocean gyres and currents; and the surface ocean mixed layer. It explores climate mode teleconnections – the atmospheric bridge, oceanic tunnel and super-gyres, and the thermal bipolar seesaw – using statistical associations and dynamical processes. Low-frequency climate variability recorded by natural climate proxies is investigated with a focus on macroweather scales and climate memory.
Paleoclimate data assimilation is reviewed with respect to convergence between proxy reconstructions and model ensembles of large-scale climate modes and circulation for the Holocene and last millennium. The chapter reviews progress in interpreting climate mode behaviour and teleconnection stationarity, particularly the North Atlantic Oscillation, the El Niño–Southern Oscillation (ENSO), the Southern Annular Mode, Zonal Wave 3, and sea ice indices. It presents approaches to resolving future problem climates using weather regime knowledge and causal networks of physical systems as applications of synoptic paleoclimatology. These include the realisation of past and future regional precipitation and winds with problem warm climates associated with tropical expansion or amplification (zonal mean Hadley Cell response) and ENSO (bias and amplitude); mid-latitude storm tracks, westerly winds, and precipitation dipoles; and polar amplification, amplified planetary waves, and extreme mid-latitude weather. Examples of causal networks and internal variability analogues that incorporate paleoweather and climate memory are applied to project future marine heat waves and cold spells.
An overview of the global energy balance, atmosphere–ocean circulation, the Hadley and Ferrell Cells, and heat and moisture budgets forms the introduction to an examination of Southern Hemisphere circulation. The chapter is a primer for paleoclimatologists working on the natural archive from the tropics to the poles. The major circulation characteristics of the Southern Hemisphere are defined in descriptive terms. Low-latitude circulation is viewed through the tropical zonal pressure gradient and Walker Circulation; tropical easterlies, near-equatorial trough, and westerlies; the Intertropical Convergence Zone over the ocean basins, the Maritime Continent, Africa, and South America; and tropical/subtropical monsoons. The mid-high latitudes are explored through the mid-latitude westerlies, circumpolar trough, Antarctic coastal easterlies and coastal-slope winds, and the annual and semi-annual oscillations in pressure and temperature. The major climate modes, El Niño–Southern Oscillation (ENSO), Indian Ocean Dipole, ENSO diversity, tropical–extratropical interactions, the Pacific–South American modes, and the Southern Annular Mode are described in terms of air–sea interactions.
Cross-shelf transport in the inner continental shelf is governed by wind, wave and tidal interactions, but the role of Langmuir circulation (LC), induced by wave–current interaction and modulated by tides, has remained under-studied in this setting. We develop a Reynolds-averaged Navier–Stokes (RANS) model incorporating the Craik–Leibovich vortex force to resolve LC, coupled with a mass-conserving undertow and oscillating along-shelf tidal currents, and compare results against field data from the Martha’s Vineyard Coastal Observatory (MVCO). Under strong wave forcing (significant wave height $H_{\textit{sig}} = 2.12\,\mathrm{m}$ and significant wave period $T_w = 5.8\,\mathrm{s}$), LC persists throughout the tidal cycle, reducing vertical shear in the tidally averaged cross-shelf velocity profile compared with simulations excluding LC. During peak tidal velocity (reaching $25\,\mathrm{cm\,s^{-1}}$ with period of $ 12.42\,\mathrm{h}$), LC is temporarily suppressed but reforms rapidly as tidal energy declines, sustaining high vertical mixing. Conversely, under weak wave forcing ( $H_{\textit{sig}} = 0.837\,\mathrm{m}$, $T_w = 4.3\,\mathrm{s}$), tidal currents persistently suppress LC, resulting in a cross-shelf undertow profile with greater vertical shear compared with strong-wave conditions. Model–observation comparisons show that only simulations including both the Craik–Leibovich vortex force and tidal forcing reproduce the observed undertow structure at MVCO. These results demonstrate that accurate prediction of cross-shelf transport at tidal and subtidal time scales requires resolving both the generation and disruption of LC by tides.