The Martian bow wave—Theory and observation

Author:

Spreiter J.R.,Rizzi A.W.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference10 articles.

1. Application of the hypersonic analog to the standing shock of Mars;Dryer;Solar Phys.,1967

2. The atmosphere of Mars analyzed by integral inversion of the Mariner IV occultation data;Fjeldbo;Planet. Space Sci.,1968

3. Solar wind and solar energetic particles: properties and interactions;Kavanagh;Rev. Geophys. Space Phys.,1970

4. Occultation experiment: results of the first direct measurement of Mars' atmosphere and ionosphere;Kliore;Science, N.Y.,1965

5. Initial results from the Mariner 4 solar plasma experiment;Lazarus;Space Res.,1967

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1. Characteristics of the Martian Magnetosphere according to the Data of the Mars 3 and Phobos 2 Satellites: Comparison with MGS and MAVEN Results;Cosmic Research;2021-11

2. Martian Bow Shock and Magnetic Pileup Boundary Models Based on an Automated Region Identification;Journal of Geophysical Research: Space Physics;2020-11

3. Annual variations in the Martian bow shock location as observed by the Mars Express mission;Journal of Geophysical Research: Space Physics;2016-11

4. Mars atmospheric losses induced by the solar wind: Comparison of observations with models;Planetary and Space Science;2015-12

5. The Magnetosphere of Mars;Physics of Solar Planetary Environments: Proceedings Of the International Symposium on Solar-Terrestrial Physics, June 7-18,1976 Boulder, Colorado Volume II;2013-03-22

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