Modeling of Diffuse Aurora due to Precipitation of H + ‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation-Reference-Cited by-同舟云学术

Modeling of Diffuse Aurora due to Precipitation of H + ‐H and SEP Electrons in the Nighttime Atmosphere of Mars: Monte Carlo Simulation and MAVEN Observation

Published:2019-11 Issue:11 Volume:124 Page:9566-9576
ISSN:2169-9380
Container-title:Journal of Geophysical Research: Space Physics
language:en
Short-container-title:J. Geophys. Res. Space Physics

Author:

Haider S. A.¹^ORCID,Masoom J.¹²^ORCID

Affiliation:

1. Planetary Sciences Division Physical Research Laboratory Ahmedabad India

2. Research Scholar, Faculty of Science Pacific Academy of Higher Education of Research University Udaipur India

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Geophysics

Link

https://onlinelibrary.wiley.com/doi/pdf/10.1029/2019JA026688

Reference47 articles.

1. Magnetic Field and Plasma Observations at Mars: Initial Results of the Mars Global Surveyor Mission

2. Discovery of an aurora on Mars

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4. CO Cameron band and CO2+ UV doublet emissions in the dayglow of Venus: Role of CO in the Cameron band production

5. Magnetic Clouds

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