EGU21-11879
https://doi.org/10.5194/egusphere-egu21-11879
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

Annual variations of Mars atmosphere, as seen by HEND data since 2002

Dmitry Golovin, Igor Mitrofanov, Maxim Litvak, Anton Sanin, and Alexey Malakhov
Dmitry Golovin et al.
  • Institute of Space Research, Moscow, Russian Federation (golovin@l503.iki.rssi.ru)

HEND (High Energy Neutron Detector) onboard NASA’s Mars Odyssey spacecraft performs measurements of neutron emission of Martian surface 2002. HEND uses 3He counters for detection of epithermal neutrons generated by Galaсtic Cosmic Rays interaction with surface and atmosphere of Mars.

Weak Martian atmosphere emits, absorbs and scatters neutrons slightly, and outgoing neutron flux on the orbit is changing depending on atmospheric density along the Martian seasons. We have analyzed the HEND data for seasonal variations of outgoing neutron flux above several areas of Mars for nine Martian annual cycles. Measured seasonal variations, presented as Ls profiles for individual years, are compared with numerically predicted profiles according to the model of Martian atmosphere.

How to cite: Golovin, D., Mitrofanov, I., Litvak, M., Sanin, A., and Malakhov, A.: Annual variations of Mars atmosphere, as seen by HEND data since 2002, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-11879, https://doi.org/10.5194/egusphere-egu21-11879, 2021.

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