EGU24-19987, updated on 11 Mar 2024
https://doi.org/10.5194/egusphere-egu24-19987
EGU General Assembly 2024
© Author(s) 2024. This work is distributed under
the Creative Commons Attribution 4.0 License.

Bursty reconnection during BepiColombo's third Mercury flyby

Ali Varsani1, Daniel Schmid1, Helmut Lammer1, Rumi Nakamura1, Kristin Pump2, Daniel Heyner2, Gunter Laky1, Harald Jeszenszky1, Gabriel Giono1, Martin Volwerk1, Anna Milillo3, Stefano Orsini3, David Fischer1, Werner Magnes1, Wolfgang Baumjohann1, and Ayako Matsuoka4
Ali Varsani et al.
  • 1Space Research Institute, Austrian Academy of Sciences, Graz, Austria
  • 2IGEP, TU Braunschweig, Germany
  • 3INAF-IAPS, Rome, Italy
  • 4Kyoto University, Japan

Mercury is known to possess a Magnetosphere that is highly responsive to the upstream Solar Wind conditions. Previous studies using MESSENGER data have contributed to understanding the dynamics of Mercury's respond to the upstream. However, the interactions between the Magnetospheric plasma and the Solar Wind is yet to be fully understood; and it is indeed one of the main focuses of the ESA/JAXA's current mission, BepiColombo. We report the observations of BepiColombo's flyby-3 at Mercury on 19th June 2023, using ion data from SERENA-PICAM and magnetic field data from MAG/MGF instruments. The preliminary analyses have given an insight into the rapidly changing plasma, at the inbound Magnetopause crossing. There is evidence that bursty reconnection could be the main contributor to such dynamic boundary.

How to cite: Varsani, A., Schmid, D., Lammer, H., Nakamura, R., Pump, K., Heyner, D., Laky, G., Jeszenszky, H., Giono, G., Volwerk, M., Milillo, A., Orsini, S., Fischer, D., Magnes, W., Baumjohann, W., and Matsuoka, A.: Bursty reconnection during BepiColombo's third Mercury flyby, EGU General Assembly 2024, Vienna, Austria, 14–19 Apr 2024, EGU24-19987, https://doi.org/10.5194/egusphere-egu24-19987, 2024.