Influence of ab initio chemistry models on simulations of the Ionian atmosphere-Reference-Cited by-同舟云学术

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Influence of ab initio chemistry models on simulations of the Ionian atmosphere

Published:2014-09 Issue: Volume:239 Page:32-38
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Parsons Neal,Levin Deborah A.,Walker Andrew C.,Moore Chris H.,Goldstein David B.,Varghese Philip L.,Trafton Laurence

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference31 articles.

1. Rarefied gas model of Io’s sublimation-driven atmosphere;Austin;Icarus,2000

2. Molecular Gas Dynamics and the Direct Simulation of Gas Flows;Bird,1994

3. Statistical collision model for Monte Carlo simulation of polyatomic gas mixture;Borgnakke;J. Comput. Phys.,1975

4. Rassvet: Backward Monte Carlo radiative transfer in spherical-shell planetary atmospheres;Gratiy;Icarus,2010

5. Multi-wavelength simulations of atmospheric radiation from Io with a 3-D spherical-shell backward Monte Carlo radiative transfer model;Gratiy;Icarus,2010

Cited by 3 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The time variation of atomic oxygen emission around Io during a volcanic event observed with Hisaki/EXCEED;Icarus;2018-01

2. Modeling of molecular nitrogen collisions and dissociation processes for direct simulation Monte Carlo;The Journal of Chemical Physics;2014-12-21

3. A post-collision internal energy model for O(3P)+SO2(X,1A1) in DSMC based on Molecular Dynamics computations;Chemical Physics;2014-10

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