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1.
Proc Natl Acad Sci U S A ; 117(26): 14764-14768, 2020 06 30.
Article in English | MEDLINE | ID: mdl-32546519

ABSTRACT

The ice shell on Enceladus, an icy moon of Saturn, exhibits strong asymmetry between the northern and southern hemispheres, with all known geysers concentrated over the south pole, even though the expected pattern of tidal forced deformation should be symmetric between the north and south poles. Using an idealized ice-evolution model, we demonstrate that this asymmetry may form spontaneously, without any noticeable a priori asymmetry (such as a giant impact or a monopole structure of geological activity), in contrast to previous studies. Infinitesimal asymmetry in the ice shell thickness due to random perturbations are found to be able to grow indefinitely, ending up significantly thinning the ice shell at one of the poles, thereby allowing fracture formation there. Necessary conditions to trigger this hemispheric symmetry-breaking mechanism are found analytically. A rule of thumb we find is that, for Galilean and Saturnian icy moons, the ice shell can undergo hemispheric symmetry breaking only if the mean shell thickness is around 10 to 30 km.

2.
Phys Rev E ; 96(4-1): 042411, 2017 Oct.
Article in English | MEDLINE | ID: mdl-29347516

ABSTRACT

Understanding the mechanisms governing population extinctions is of key importance to many problems in ecology and evolution. Stochastic factors are known to play a central role in extinction, but the interactions between a population's demographic stochasticity and environmental noise remain poorly understood. Here we model environmental forcing as a stochastic fluctuation between two states, one with a higher death rate than the other. We find that, in general, there exists a rate of fluctuations that minimizes the mean time to extinction, a phenomenon previously dubbed "resonant activation." We develop a heuristic description of the phenomenon, together with a criterion for the existence of resonant activation. Specifically, the minimum extinction time arises as a result of the system approaching a scenario wherein the severity of rare events is balanced by the time interval between them. We discuss our findings within the context of more general forms of environmental noise and suggest potential applications to evolutionary models.


Subject(s)
Extinction, Biological , Models, Biological , Computer Simulation , Environment , Population Dynamics , Stochastic Processes , Time Factors
3.
J Geophys Res Oceans ; 120(6): 4129-4150, 2015 Jun.
Article in English | MEDLINE | ID: mdl-26937328

ABSTRACT

Trichodesmium abundance was elevated in certain cyclonic and anticyclonic eddiesEnhancement in cyclonic eddies could be driven by Ekman convergenceAnticyclonic eddies with elevated abundance were anomalously fresh.

4.
Science ; 327(5972): 1509-11, 2010 Mar 19.
Article in English | MEDLINE | ID: mdl-20185684

ABSTRACT

Spatial diversity gradients are a pervasive feature of life on Earth. We examined a global ocean circulation, biogeochemistry, and ecosystem model that indicated a decrease in phytoplankton diversity with increasing latitude, consistent with observations of many marine and terrestrial taxa. In the modeled subpolar oceans, seasonal variability of the environment led to competitive exclusion of phytoplankton with slower growth rates and lower diversity. The relatively weak seasonality of the stable subtropical and tropical oceans in the global model enabled long exclusion time scales and prolonged coexistence of multiple phytoplankton with comparable fitness. Superimposed on the decline in diversity seen from equator to pole were "hot spots" of enhanced diversity in some regions of energetic ocean circulation, which reflected lateral dispersal.


Subject(s)
Biodiversity , Ecosystem , Phytoplankton , Seawater , Biomass , Climate , Environment , Geography , Models, Biological , Oceans and Seas , Phytoplankton/growth & development , Phytoplankton/physiology , Population Dynamics , Seasons
5.
Philos Trans R Soc Lond B Biol Sci ; 357(1421): 657-66, 2002 May 29.
Article in English | MEDLINE | ID: mdl-12079527

ABSTRACT

Three different lattice-based models for antagonistic ecological interactions, both nonlinear and stochastic, exhibit similar power-law scalings in the geometry of clusters. Specifically, cluster size distributions and perimeter-area curves follow power-law scalings. In the coexistence regime, these patterns are robust: their exponents, and therefore the associated Korcak exponent characterizing patchiness, depend only weakly on the parameters of the systems. These distributions, in particular the values of their exponents, are close to those reported in the literature for systems associated with self-organized criticality (SOC) such as forest-fire models; however, the typical assumptions of SOC need not apply. Our results demonstrate that power-law scalings in cluster size distributions are not restricted to systems for antagonistic interactions in which a clear separation of time-scales holds. The patterns are characteristic of processes of growth and inhibition in space, such as those in predator-prey and disturbance-recovery dynamics. Inversions of these patterns, that is, scalings with a positive slope as described for plankton distributions, would therefore require spatial forcing by environmental variability.


Subject(s)
Ecosystem , Food Chain , Models, Biological , Animals , Bivalvia , Cluster Analysis
6.
Chaos ; 4(2): 355-367, 1994 Jun.
Article in English | MEDLINE | ID: mdl-12780110

ABSTRACT

Solitary wave or isolated eddy models are often invoked to explain the longevity of strong nonlinear features in oceans and atmospheres. But when we look at the physics in detail, we find that models of isolated eddies often hinge either on an oversimplification of the dynamics or on constraints which are not appropriate for the observed eddies. In a more complete model, as this study demonstrates, rings (and probably other nonlinear geophysical eddies as well) will interact with their surroundings via Rossby wave radiation, primarily in the barotropic mode. Such wave generation leads to a slow decay of the eddy as energy leaks into the wave field.

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