EGU25-6945, updated on 14 Mar 2025
https://doi.org/10.5194/egusphere-egu25-6945
EGU General Assembly 2025
© Author(s) 2025. This work is distributed under
the Creative Commons Attribution 4.0 License.
Oral | Monday, 28 Apr, 11:30–11:40 (CEST)
 
Room 1.85/86
Observations from the Mercury Electron Analyzer onboard BepiColombo during its sixth Mercury flyby
Nicolas André1,2, Jean-André Sauvaud2, Yoshifumi Saito3, Mathias Rojo2, Sae Aizawa4, Andrei Fedorov2, Emmanuel Penou2, Alain Barthe5, Shoichiro Yokota6, Zdenek Nemecek7, Jana Safrankova7, Maria Federica Marcucci8, Zhi-Yang Liu2, Moa Persson9, Lina Hadid4, Dominique Delcourt4, Yuki Harada10, Markus Fraenz11, Norbert Krupp11, and Go Murakami3
Nicolas André et al.
  • 1Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France (nicolas.andre@isae-supaero.fr)
  • 2IRAP-CNRS-CNES-Toulouse University, Toulouse, France
  • 3Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara, Japan
  • 4LPP, CNRS, Observatoire de Paris, Sorbonne Université, Université Paris Saclay, École polytechnique, Institut Polytechnique de Paris, Palaiseau, France
  • 5AKKODIS, Toulouse, France
  • 6Department of Earth and Space Science, Graduate School of Science, Osaka University, Osaka, Japa
  • 7Faculty of Mathematics and Physics, Charles University, Prague, Czech Republic
  • 8INAF - Istituto di Astrofisica e Planetologia Spaziali, Roma, Italy
  • 9Swedish Institute of Space Physics, Uppsala, Sweden
  • 10Department of Geophysics, Graduate School of Science, Kyoto University, Kyoto, Japan
  • 11Max Planck Institute for Solar System Research (MPS), Göttingen, Germany

On 8 January 2025, the ESA/JAXA BepiColombo mission flew by Mercury for the sixth time at an altitude of 295 km. The spacecraft took on a unique route through Mercury’s magnetic and particle environment, crossing the equator opposite the Sun on Mercury’s night side before flying over the planet’s north pole. During eclipse, in the cold shadow of the planet, as well as above the northern pole the spacecraft passed through regions where charged particles precipitate from the planet’s magnetic tail and from the solar wind towards its surface. We will detail the original electron observations obtained by the Mercury Electron Analyzer during Mercury’s sixth flyby, and compare and contrast them with electron observations obtained during previous BepiColombo flybys. All together, these new observations will provide new insights into the diversity of structures observed in these regions and the underlying mechanisms responsible for their formation and dynamics.

 

How to cite: André, N., Sauvaud, J.-A., Saito, Y., Rojo, M., Aizawa, S., Fedorov, A., Penou, E., Barthe, A., Yokota, S., Nemecek, Z., Safrankova, J., Marcucci, M. F., Liu, Z.-Y., Persson, M., Hadid, L., Delcourt, D., Harada, Y., Fraenz, M., Krupp, N., and Murakami, G.: Observations from the Mercury Electron Analyzer onboard BepiColombo during its sixth Mercury flyby, EGU General Assembly 2025, Vienna, Austria, 27 Apr–2 May 2025, EGU25-6945, https://doi.org/10.5194/egusphere-egu25-6945, 2025.