Convective dynamics and disequilibrium chemistry in the atmospheres of giant planets and brown dwarfs

Disequilibrium chemical processes have a large effect upon the spectra of substellar objects. To study these effects, dynamical disequilibrium has been parameterized using the quench and eddy diffusion approximations, but little work has been done to explore how these approximations perform under re...

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Veröffentlicht in:	arXiv.org 2018-02
Hauptverfasser:	Bordwell, Baylee, Brown, Benjamin P, Oishi, Jeffrey S
Format:	Artikel
Sprache:	eng
Schlagworte:	Atmospheric models Brown dwarf stars Chemical reactions Compressibility Computational fluid dynamics Computer simulation Direct numerical simulation Fluid flow Hydrodynamics Mathematical models Organic chemistry Parameterization Physics - Earth and Planetary Astrophysics Planetary atmospheres Predictions Reaction kinetics Scale height Tracers
Online-Zugang:	Volltext
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