Semkova Jordanka, Koleva Rositza, Benghin Victor, Krastev Krasimir, Matviichuk Yuri, Tomov Borislav, Maltchev Stephan, Dachev Tsvetan, Bankov Nikolay, Mitrofanov Igor, Malakhov Alexey, Golovin Dmitry, Litvak Maxim, Sanin Anton, Kozyrev Alexander, Mokrousov Maxim, Nikiforov Sergey, Lisov Denis, Anikin Artem, Shurshakov Vyacheslav, Drobyshev Sergey, Gopalswamy Nat
Space Research and Technology Institute, Bulgarian Academy of Sciences, Sofia, Bulgaria.
Space Research and Technology Institute, Bulgarian Academy of Sciences, Sofia, Bulgaria.
Life Sci Space Res (Amst). 2023 Nov;39:106-118. doi: 10.1016/j.lssr.2023.03.006. Epub 2023 Mar 31.
The dosimeter Liulin-MO for measuring the radiation environment onboard the ExoMars Trace Gas Orbiter (TGO) is a module of the Fine Resolution Epithermal 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, particle flux is 3.3 ± 0.17 cms, dose equivalent rate is 72.3 ± 14.4 µSv h. 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.
用于测量火星微量气体轨道器(TGO)上辐射环境的“柳林-MO”剂量计是精细分辨率超热中子探测器(FREND)的一个模块。本文展示了“柳林-MO”在2018年5月至2022年6月期间为火星科学轨道上的火星微量气体轨道器提供的带电粒子通量、剂量率测量结果以及剂量当量率估算结果。测量期涵盖了第24太阳活动周太阳活动的下降和极小阶段以及第25太阳活动周的上升阶段。比较了在太阳活动不同阶段获得的银河宇宙射线(GCR)的辐射值。GCR剂量率和通量的最高值出现在2020年3月至8月。在第24太阳活动周极小期以及向第25太阳活动周过渡期间,GCR的剂量率为15.9±1.6微戈瑞/小时,粒子通量为3.3±0.17厘米²,剂量当量率为72.3±14.4微希沃特/小时。自2020年9月起,GCR的剂量率和通量下降。特别关注了2021年7月、9月和10月、2022年2月和3月太阳高能粒子(SEP)事件的观测以及它们在相应时期对火星微量气体轨道器辐射环境的影响。2022年2月15日至19日的SEP事件是我们数据中观测到的最强事件。该事件期间的SEP剂量为(硅中)13.8±1.4毫戈瑞,SEP剂量当量为21.9±4.4毫希沃特。在火星轨道记录的SEP事件与太阳和日球层探测器(SOHO)及日地关系天文台A(STEREO A)日冕仪观测到的日冕物质抛射(CME)有关。比较了2022年2月15日至19日事件期间“柳林-MO”、FREND中子探测器以及火星奥德赛号高能中子探测器(HEND)测量的计数率时间剖面。所获得的数据对于了解火星周围辐射环境、关乎未来前往该行星的载人及机器人飞行而言至关重要。2021年7月至2022年3月火星轨道SEP事件的数据有助于详细了解火星位于太阳与地球相对一侧时的太阳活动情况。