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BepiColombo Mio Observations of Low-Energy Ions During the First Mercury Flyby: Initial Results

  • Yuki Harada
  • , Sae Aizawa
  • , Yoshifumi Saito
  • , Nicolas André
  • , Moa Persson
  • , Dominique Delcourt
  • , Lina Z. Hadid
  • , Markus Fraenz
  • , Shoichiro Yokota
  • , Andréi Fedorov
  • , Wataru Miyake
  • , Emmanuel Penou
  • , Alain Barthe
  • , Jean André Sauvaud
  • , Bruno Katra
  • , Shoya Matsuda
  • , Go Murakami
  • Department of Astronomy, Graduate School of Science, Kyoto University
  • Centre National d'études Spatiales
  • ISAS/JAXA
  • Sorbonne Université
  • Max-Planck-Institut für Sonnensystemforschung
  • Osaka University
  • Tokai University
  • Kanazawa University

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We present initial results of low-energy ion observations from BepiColombo's first Mercury flyby. Unprecedentedly high time resolution measurements of low energy ions at Mercury by BepiColombo Mio reveal rapid (a few seconds) and large (1–2 orders of magnitude) fluctuations of ion flux around the magnetopause and within the magnetosphere. Around the magnetic equator in the pre-midnight magnetotail, Mio observed plasma sheet ions consistent with previous observations. In the midnight magnetotail near the closest approach, Mio observed the co-existence of high-energy (∼keV/q) and low-energy (<∼300 eV/q) ion components. The low-energy component is inferred to be cold with a temperature well below 100 eV and have a major contribution to the total density as opposed to previously reported cold tenuous ions. Future observations by Mio will provide insights into the sources, transport, and acceleration of the newly identified ion components.

langue originaleAnglais
Numéro d'articlee2022GL100279
journalGeophysical Research Letters
Volume49
Numéro de publication17
Les DOIs
étatPublié - 16 sept. 2022
Modification externeOui

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