{"title":"The solar particle event at Mars on 2024 May 20: neutron component of the radiation environment","authors":"Igor Mitrofanov , Maxim Litvak , Anton Sanin , Dmitry Golovin , Sergey Nikiforov , Maya Djachkova , Artem Anikin , Nikita Lukyanov , Jordanka Semkova , Yuri Matviichuk","doi":"10.1016/j.actaastro.2025.05.043","DOIUrl":null,"url":null,"abstract":"<div><div>This paper presents the observational findings for the most powerful solar particle event (SPE) on Mars in the current 25th solar cycle, based on surface (DAN/Curiosity) and orbital (HEND/Mars Odyssey) measurements. The numerical modelling of SPE proton interaction with the atmosphere and Martian surface showed that the computational results are in good agreement with the experimental data. The neutron component of the radiation background in orbit and on the surface was evaluated near the SPE maximum. The integral neutron dose on the Martian surface during the entire SPE was estimated as 600 μSv, which equals the dose received during ∼11 days in quiet Sun environment. The obtained data were extrapolated to more powerful solar events known from the history of observation. The Carrington event was used as an example. For such a hypothetical SPE, the total neutron dose may achieve as high as 240 mSv. It is 1.6 times higher than annual dose limit allowed for astronauts in the NASA ORION project.</div></div>","PeriodicalId":44971,"journal":{"name":"Acta Astronautica","volume":"234 ","pages":"Pages 734-741"},"PeriodicalIF":3.1000,"publicationDate":"2025-05-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Acta Astronautica","FirstCategoryId":"5","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S009457652500325X","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"ENGINEERING, AEROSPACE","Score":null,"Total":0}
引用次数: 0
Abstract
This paper presents the observational findings for the most powerful solar particle event (SPE) on Mars in the current 25th solar cycle, based on surface (DAN/Curiosity) and orbital (HEND/Mars Odyssey) measurements. The numerical modelling of SPE proton interaction with the atmosphere and Martian surface showed that the computational results are in good agreement with the experimental data. The neutron component of the radiation background in orbit and on the surface was evaluated near the SPE maximum. The integral neutron dose on the Martian surface during the entire SPE was estimated as 600 μSv, which equals the dose received during ∼11 days in quiet Sun environment. The obtained data were extrapolated to more powerful solar events known from the history of observation. The Carrington event was used as an example. For such a hypothetical SPE, the total neutron dose may achieve as high as 240 mSv. It is 1.6 times higher than annual dose limit allowed for astronauts in the NASA ORION project.
期刊介绍:
Acta Astronautica is sponsored by the International Academy of Astronautics. Content is based on original contributions in all fields of basic, engineering, life and social space sciences and of space technology related to:
The peaceful scientific exploration of space,
Its exploitation for human welfare and progress,
Conception, design, development and operation of space-borne and Earth-based systems,
In addition to regular issues, the journal publishes selected proceedings of the annual International Astronautical Congress (IAC), transactions of the IAA and special issues on topics of current interest, such as microgravity, space station technology, geostationary orbits, and space economics. Other subject areas include satellite technology, space transportation and communications, space energy, power and propulsion, astrodynamics, extraterrestrial intelligence and Earth observations.