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Published December 28, 2022 | Version version 0
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Direct evidence of substorm-related impulsive injections of electrons at Mercury

  • 1. 1IRAP, CNRS-UPS-CNES, Toulouse, France, Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan, University of Pisa, Pisa, Italy
  • 2. Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan
  • 3. IRAP, CNRS-UPS-CNES, Toulouse, France
  • 4. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan
  • 5. Swedish Institute of Space Physics, Kiruna SE 98192, Sweden
  • 6. LPP-CNRS-Sorbonne Université-Ecole Polytechnique, Paris, France Laboratoire de Physique des Plasmas (LPP), CNRS, Observatoire de Paris, Sorbonne Université, Université Paris Saclay, École polytechnique, Institut Polytechnique de Paris, 91120 Palaiseau, France
  • 7. Department of Earth and Space Science, Graduate School of Science, Osaka University, Japan
  • 8. Tokai University, Kanagawa, Japan
  • 9. Max-Planck-Institute for Solar System Research, Göttingen, Germany
  • 10. Kanazawa University, Kanazawa, Japan

Description

This data set includes electron energy-time spectrograms obtained by MEA1 and MEA2 in units of differential energy flux (eV/cm^2/s/sr/eV) and energetic neutral atoms obtained by ENA in counts during BepiColombo Mio's first Mercury flyby. The data are uncalibrated, thus to properly use these data, contacting PI teams is highly recommended.

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