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Jonathan L. Mitchell

Researcher at University of California, Los Angeles

Publications -  71
Citations -  2169

Jonathan L. Mitchell is an academic researcher from University of California, Los Angeles. The author has contributed to research in topics: Titan (rocket family) & Hadley cell. The author has an hindex of 25, co-authored 64 publications receiving 1852 citations. Previous affiliations of Jonathan L. Mitchell include California NanoSystems Institute & University of Illinois at Chicago.

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Improved Cosmological Constraints from Gravitational Lens Statistics

TL;DR: In this paper, the authors combine the cosmic lens All-Sky Survey (CLASS) with new Sloan Digital Sky Survey (SDSS) data on the local velocity dispersion distribution function of E/S0 galaxies, to derive lens statistics constraints on the cosmological parameters.
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The drying of Titan's dunes: Titan's methane hydrology and its impact on atmospheric circulation

TL;DR: In this paper, the authors explore the effect of a finite reservoir of methane on Titan's atmospheric circulation, precipitation patterns, and surface methane content and develop a soil model that accounts for the methane cycle in the surface-atmosphere system, and implement this surface model in a two-dimensional model of the Titan's atmosphere.
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The dynamics behind Titan's methane clouds.

TL;DR: Results of an axisymmetric global circulation model of Titan with a simplified suite of atmospheric physics forced by seasonally varying insolation find clouds at the solsticial pole are found to be a robust feature of Titan's dynamics, whereas isolated midlatitude clouds are present exclusively in a variety of moist dynamical regimes.
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Generalized milankovitch cycles and long-term climatic habitability

TL;DR: In this article, the authors revisited one-dimensional energy balance climate models as tools for probing possible climates of exoplanets, and introduced a simple algorithm to treat the melting of the ice layer on a globally frozen planet.
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The transition to superrotation in terrestrial atmospheres

TL;DR: In this paper, the transition to superrotation occurs under conditions in which equatorward propagating Rossby waves generated by baroclinic instability at intermediate and high latitudes are suppressed, which will occur when the deformation radius exceeds the planetary radius.