- 1Institut Supérieur de l'Aéronautique et de l'Espace (ISAE-SUPAERO), Université de Toulouse, Toulouse, France
- 2IRAP, CNRS, CNES, Université de Toulouse, Toulouse, France
- *A full list of authors appears at the end of the abstract
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.
Mathias Rojo (2), Camille Coustillet (2), Jean-André Sauvaud (2), Yoshifumi Saito (3), Sae Aizawa (4), Andrei Fedorov (2), Emmanuel Penou (2), Alain Barthe (2), Shoichiro Yokota (5), Zdenek Nemecek (6), Jana Safrankova (6), Maria Federica Marcucci (7), Zhi-Yang Liu (2), Moa Persson (8), Lina Hadid (4), Dominique Delcourt (4), Yuki Harada (9), Markus Fraenz (10), Norbert Krupp (10), and Go Murakami (3)
How to cite: André, N. and the MEA-MPPE Team: Observations from the Mercury Electron Analyzer onboard BepiColombo during its sixth Mercury flyby , EPSC-DPS Joint Meeting 2025, Helsinki, Finland, 7–12 Sep 2025, EPSC-DPS2025-1442, https://doi.org/10.5194/epsc-dps2025-1442, 2025.