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Observation of the Radiation Environment and Solar Energetic Particle Events in Mars Orbit in May 2018- June 2022Epithermal Neutron Detector (FREND). Here we present results from measurements of the charged particle fluxes, dose rates and estimation of dose equivalent rates at ExoMars TGO Mars science orbit, provided by Liulin-MO from May 2018 to June 2022. The period of measurements covers the declining and minimum phases of the solar activity in 24th solar cycle and the rising phase of the 25th cycle. Compared are the radiation values of the galactic cosmic rays (GCR) obtained during the different phases of the solar activity. The highest values of the dose rate and flux from GCR are registered from March to August 2020. At the minimum of 24th and transition to 25th solar cycle the dose rate from GCR is 15.9 ± 1.6 µGy h−1, particle flux is 3.3 ± 0.17 cm−2 s−1, dose equivalent rate is 72.3 ± 14.4 µSv h−1. Since September 2020 the dose rate and flux of GCR decrease. Particular attention is drawn to the observation of the solar energetic particle (SEP) events in July, September and October 2021, February and March 2022 as well as their effects on the radiation environment on TGO during the corresponding periods. The SEP event during15–19 February 2022 is the most powerful event observed in our data. The SEP dose during this event is 13.8 ± 1.4 mGy (in Si), the SEP dose equivalent is 21.9 ± 4.4 mSv. SEP events recorded in Mars orbit are related to coronal mass ejections (CME) observed by SOHO and STEREO A coronagraphs. Compared are the time profiles of the count rates measured by Liulin-MO, the neutron detectors of FREND and neutron detectors of the High Energy Neutron Detector (HEND) aboard Mars Odyssey during 15–19 February 2022 event. The data obtained is important for the knowledge of the radiation environment around Mars, regarding future manned and robotic flights to the planet. The data for SEP events in Mars orbit during July 2021-March 2022 contribute to the details on the solar activity at a time when Mars is on the opposite side of the Sun from Earth.
Document ID
20230014497
Acquisition Source
Goddard Space Flight Center
Document Type
Reprint (Version printed in journal)
Authors
Jordanka Semkova
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Rositza Koleva
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Victor Benghin
(Institute of Biomedical Problems Moscow, Russia)
Krasimir Krastev
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Yuri Matviichuk
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Borislav Tomov
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Stephan Maltchev
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Tsvetan Dachev
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Nikolay Bankov
(Bulgarian Academy of Sciences Sofia, Bulgaria)
Igor Mitrofanov
(Space Research Institute Moscow, Russia)
Alexey Malakhov
(Space Research Institute Moscow, Russia)
Dmitry Golovin
(Space Research Institute Moscow, Russia)
Maxim Litvak
(Space Research Institute Moscow, Russia)
Anton Sanin
(Space Research Institute Moscow, Russia)
Alexander Kozyrev
(Space Research Institute Moscow, Russia)
Maxim Mokrousov
(Space Research Institute Moscow, Russia)
Sergey Nikiforov
(Space Research Institute Moscow, Russia)
Denis Lisov
(Space Research Institute Moscow, Russia)
Artem Anikin
(Space Research Institute Moscow, Russia)
Vyacheslav Shurshakov
(Institute of Biomedical Problems Moscow, Russia)
Sergey Drobyshev
(Institute of Biomedical Problems Moscow, Russia)
Nat Gopalswamy
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
October 5, 2023
Publication Date
March 31, 2023
Publication Information
Publication: Life Sciences in Space Research
Publisher: Elsevier
Volume: 39
Issue Publication Date: November 1, 2023
ISSN: 0024-3205
Subject Category
Life Sciences (General)
Space Sciences (General)
Funding Number(s)
WBS: 937818.01.02.04
CONTRACT_GRANT: J-090011
CONTRACT_GRANT: 4000133961/21/NL/SC
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