Theory for planetary exospheres: III. Radiation pressure effect on the Circular Restricted Three Body Problem and its implication on planetary atmospheres-Reference-Cited by-同舟云学术

Theory for planetary exospheres: III. Radiation pressure effect on the Circular Restricted Three Body Problem and its implication on planetary atmospheres

Published:2016-12 Issue: Volume:280 Page:415-423
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Beth A.^ORCID,Garnier P.,Toublanc D.,Dandouras I.,Mazelle C.

Funder

CNES

STFC

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference37 articles.

1. Abel, N. H., 1824. Mémoire sur les équations algébriques, oùon démontre l’impossibilité de la résolution de l’équation générale du cinquième degré.

2. Theory for planetary exospheres: I. Radiation pressure effect on dynamical trajectories;Beth;Icarus,2016

3. Theory for planetary exospheres: II. Radiation pressure effect on exospheric density profiles;Beth;Icarus,2016

4. Analytic exosphere models for geocoronal applications;Bishop;Planet. Space Sci.,1991

5. Radiation pressure dynamics in planetary exospheres: A natural framework;Bishop;Icarus,1989

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