A2 Vertaisarvioitu katsausartikkeli tieteellisessä lehdessä
The BepiColombo Environment Radiation Monitor, BERM
Tekijät: Pinto Marco, Sanchez-Cano Beatriz, Moissl Richard, Benkhoff Johannes, Cardoso Carlota, Goncalves Patrícia, Assis Pedro, Vainio Rami, Oleynik Philipp, Lehtolainen Arto, Grande Manuel, Marques Arlindo
Kustantaja: SPRINGER
Julkaisuvuosi: 2022
Journal: Space Science Reviews
Tietokannassa oleva lehden nimi: SPACE SCIENCE REVIEWS
Lehden akronyymi: SPACE SCI REV
Artikkelin numero: 54
Vuosikerta: 218
Numero: 7
Sivujen määrä: 21
ISSN: 0038-6308
eISSN: 1572-9672
DOI: https://doi.org/10.1007/s11214-022-00922-2
Verkko-osoite: https://link.springer.com/article/10.1007/s11214-022-00922-2
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/176692830
The 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.
Ladattava julkaisu This is an electronic reprint of the original article. |  |
