C+ 133.5 nm Emission Mechanisms on Mars Revealed by the MAVEN Observations

C+ 133.5 nm Emission Mechanisms on Mars Revealed by the MAVEN Observations

C ^+ emission is generated by electron impact, dissociative ionization, photoionization, and resonant scattering with carbon-related atoms, molecules, and ions in the Martian ionosphere and thermosphere. The contribution of each mechanism to the emission, however, has not been elucidated due to the...

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Bibliographic Details
Main Authors: Shotaro Sakai, Hiromu Nakagawa, Justin Deighan, Sonal K. Jain, Kei Masunaga, Fuminori Tsuchiya, Naoki Terada, Majd Mayyasi, Nicholas M. Schneider, David L. Mitchell, Christian Mazelle, Mehdi Benna, Robert J. Lillis, Go Murakami, Shannon M. Curry, Kanako Seki
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Mars
Ultraviolet spectroscopy
Extreme ultraviolet astronomy
Solar system terrestrial planets
Online Access:https://doi.org/10.3847/1538-4357/ad8e35
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https://doi.org/10.3847/1538-4357/ad8e35

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