Global S&T Development Trend Analysis Platform of Resources and Environment
DOI | 10.1029/2018GL077760 |
Analysis of the Radiation Hazard Observed by RAD on the Surface of Mars During the September 2017 Solar Particle Event | |
Zeitlin, C.1; Hassler, D. M.2; Guo, J.3; Ehresmann, B.2; Wimmer-Schweingruber, R. F.3; Rafkin, S. C. R.2; von Forstner, J. L. Freiherr3; Lohf, H.3; Berger, T.4; Matthiae, D.4; Reitz, G.4 | |
2018-06-28 | |
发表期刊 | GEOPHYSICAL RESEARCH LETTERS
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ISSN | 0094-8276 |
EISSN | 1944-8007 |
出版年 | 2018 |
卷号 | 45期号:12页码:5845-5851 |
文章类型 | Article |
语种 | 英语 |
国家 | USA; Germany |
英文摘要 | We report dosimetric quantities measured by the Mars Science Laboratory Radiation Assessment Detector (RAD) on the surface of Mars during the 10-12 September 2017 solar particle event. Despite 23g/cm(2) of CO2 shielding provided by the atmosphere above RAD, dose rates rose above background galactic cosmic ray levels by factors of 2 to 3 over the course of several hours and leveled off at sustained peak rates for about 12hr before declining over the following 36hr. As the solar particle event flux was gradually declining, a shock front reached Mars and caused a sudden drop of about 15% in instantaneous dose rates. No solar particles followed the shock arrival, and the magnetic shielding of galactic cosmic rays by the shock reduced their intensity to levels below those seen before the start of the event. This event is the largest seen to date by RAD on Mars. Plain Language Summary We report the radiation dose rate on the surface of Mars measured by the Radiation Assessment Detector (RAD) aboard the Curiosity rover before, during, and after the solar energetic particle (SEP) event of 10-12 September 2017. Future astronauts exploring Mars will be at risk from SEP events, which occur sporadically and often with little warning, as well as from galactic cosmic rays, which are a continuous source of radiation dose and which generally have higher energies than SEPs. The event described here was the largest so far observed by RAD in more than five years on Mars. Although the atmosphere of Mars is only about 1-2% as thick as Earth's, it provides a measure of shielding against solar particles, most of which are protons with energies insufficient to penetrate Mars' atmosphere and reach the surface. But in this event, RAD saw a clear increase in dose rates; the peak dose rate was nearly three times above galactic cosmic ray levels measured prior to the event. Though the increase was rapid and lasted for three days, it was too small to represent a risk to the health of an astronaut receiving it. Much larger SEP events are possible and could cause problematic doses. |
英文关键词 | solar event radiation hazard Mars surface |
领域 | 气候变化 |
收录类别 | SCI-E |
WOS记录号 | WOS:000438499100005 |
WOS关键词 | ASSESSMENT DETECTOR RAD |
WOS类目 | Geosciences, Multidisciplinary |
WOS研究方向 | Geology |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://119.78.100.173/C666/handle/2XK7JSWQ/28967 |
专题 | 气候变化 |
作者单位 | 1.Leidos Innovat Corp, Houston, TX 77042 USA; 2.Southwest Res Inst, Boulder, CO USA; 3.Univ Kiel, Dept Phys, Kiel, Germany; 4.German Aerosp Ctr, Cologne, Germany |
推荐引用方式 GB/T 7714 | Zeitlin, C.,Hassler, D. M.,Guo, J.,et al. Analysis of the Radiation Hazard Observed by RAD on the Surface of Mars During the September 2017 Solar Particle Event[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(12):5845-5851. |
APA | Zeitlin, C..,Hassler, D. M..,Guo, J..,Ehresmann, B..,Wimmer-Schweingruber, R. F..,...&Reitz, G..(2018).Analysis of the Radiation Hazard Observed by RAD on the Surface of Mars During the September 2017 Solar Particle Event.GEOPHYSICAL RESEARCH LETTERS,45(12),5845-5851. |
MLA | Zeitlin, C.,et al."Analysis of the Radiation Hazard Observed by RAD on the Surface of Mars During the September 2017 Solar Particle Event".GEOPHYSICAL RESEARCH LETTERS 45.12(2018):5845-5851. |
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