The BepiColombo Environment Radiation Monitor, BERM

dc.contributor.authorPinto Marco
dc.contributor.authorSanchez-Cano Beatriz
dc.contributor.authorMoissl Richard
dc.contributor.authorBenkhoff Johannes
dc.contributor.authorCardoso Carlota
dc.contributor.authorGoncalves Patrícia
dc.contributor.authorAssis Pedro
dc.contributor.authorVainio Rami
dc.contributor.authorOleynik Philipp
dc.contributor.authorLehtolainen Arto
dc.contributor.authorGrande Manuel
dc.contributor.authorMarques Arlindo
dc.contributor.organizationfi=avaruustutkimuslaboratorio|en=Space Research Laboratory|
dc.contributor.organization-code1.2.246.10.2458963.20.47833719389
dc.converis.publication-id176692830
dc.converis.urlhttps://research.utu.fi/converis/portal/Publication/176692830
dc.date.accessioned2022-11-02T13:13:29Z
dc.date.available2022-11-02T13:13:29Z
dc.description.abstractThe BepiColombo Environment Radiation Monitor (BERM) on board the European Space Agency's Mercury Planetary Orbiter (MPO), is designed to measure the radiation environment encountered by BepiColombo. The instrument measures electrons with energies from similar to 150 keV to similar to 10 MeV, protons with energies from similar to 1.5 MeV to similar to 100 MeV, and heavy ions with Linear Energy Transfer from 1 to 50 MeV.mg(-1).cm(2). BERM is operated continuously, being responsible for monitoring the radiation levels during all phases of the mission, including the cruise, the planetary flybys of Earth, Venus and Mercury, and the Hermean environment. In this paper, we describe the scientific objectives, instrument design and calibration, and the in-flight scientific performance of BERM. Moreover, we provide the first scientific results obtained by BERM during the BepiColombo flyby of Earth in April 2020, and after the impact of a solar energetic particle event during the cruise phase in May 2021. We also discuss the future plans of the instrument including synergies with other instruments on the BepiColombo and on other missions.
dc.identifier.eissn1572-9672
dc.identifier.jour-issn0038-6308
dc.identifier.olddbid189890
dc.identifier.oldhandle10024/172984
dc.identifier.urihttps://www.utupub.fi/handle/11111/29612
dc.identifier.urlhttps://link.springer.com/article/10.1007/s11214-022-00922-2
dc.identifier.urnURN:NBN:fi-fe2022110164024
dc.language.isoen
dc.okm.affiliatedauthorVainio, Rami
dc.okm.affiliatedauthorOleynik, Philipp
dc.okm.discipline115 Astronomy and space scienceen_GB
dc.okm.discipline115 Avaruustieteet ja tähtitiedefi_FI
dc.okm.internationalcopublicationinternational co-publication
dc.okm.internationalityInternational publication
dc.okm.typeA2 Scientific Article
dc.publisherSPRINGER
dc.publisher.countryNetherlandsen_GB
dc.publisher.countryAlankomaatfi_FI
dc.publisher.country-codeNL
dc.relation.articlenumber54
dc.relation.doi10.1007/s11214-022-00922-2
dc.relation.ispartofjournalSpace Science Reviews
dc.relation.issue7
dc.relation.volume218
dc.source.identifierhttps://www.utupub.fi/handle/10024/172984
dc.titleThe BepiColombo Environment Radiation Monitor, BERM
dc.year.issued2022

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