2021
DOI: 10.1016/j.icarus.2020.114264
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Results from radiation environment measurements aboard ExoMars Trace Gas Orbiter in Mars science orbit in May 2018–December 2019

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Cited by 10 publications
(7 citation statements)
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“…Recent studies have also analyzed data from Mars Express [Knutsen et al, 2021]. The ExoMars TGO spacecraft launched in April 2016 carries the FREND instrument, one module of the latter being the Liulin-MO dosimeter [Mitrofanov et al, 2018], that has provided and providing in-situ measurements of the radiation environment during the TGO interplanetary travel and in Martian orbit [Semkova et al, , 2021. Since May 2018 Liulin-MO investigates the radiation conditions in Mars Science Orbit (MSO).…”
Section: Discussionmentioning
confidence: 99%
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“…Recent studies have also analyzed data from Mars Express [Knutsen et al, 2021]. The ExoMars TGO spacecraft launched in April 2016 carries the FREND instrument, one module of the latter being the Liulin-MO dosimeter [Mitrofanov et al, 2018], that has provided and providing in-situ measurements of the radiation environment during the TGO interplanetary travel and in Martian orbit [Semkova et al, , 2021. Since May 2018 Liulin-MO investigates the radiation conditions in Mars Science Orbit (MSO).…”
Section: Discussionmentioning
confidence: 99%
“…Since September 2020 a decrease of the dose rates and fluxes is seen corresponding to the increasing phase of the 25 th solar cycle. [Semkova et al, 2021] Until July 2021 the dosimeter measured the dosimetric parameters of GCR. No solar particle events (SPE) were registered.…”
Section: Particle Fluxes and Dose Rates From Gcr In The Period May 20...mentioning
confidence: 99%
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“…TGO was inserted into Mars science orbit (circular orbit with about 400 km altitude, 74 0 inclination, ~ 2 hours orbit period) on 9 April 2018. On 16 April 2018 Liulin-MO was switched on and since then operates almost continuously (Semkova et al, 2021). Тhe relatively short period of our data obtained in Mars orbit (three years) allows us to trace only part of the 11-year variation of galactic cosmic rays, but it allows us to observe short term variations in the charged particles flux, caused by large-scale disturbances of the solar wind (Forbush effect).…”
Section: Introductionmentioning
confidence: 94%
“…[8][9][10] Based on the data recorded by the gamma-ray spectrometer and neutron spectrometer in previous Mars detectors, researchers have studied the variation, distribution, and even the dose of Mars orbit. [11][12][13][14][15] However, on-orbit electrical performance degradation of solar array induced by the fixed charge particles radiation in Mars orbit has not been seen.…”
Section: Introductionmentioning
confidence: 99%