Journal
NATURE COMMUNICATIONS
Volume 13, Issue 1, Pages -Publisher
NATURE PORTFOLIO
DOI: 10.1038/s41467-022-34988-x
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Funding
- Italian Space Agency (ASI)
- Italian National Institute of Astrophysics (INAF) [2018-8-HH.0]
- SERENA Science Operations (EXPRO), ESA [C4000119196/16/ES/JD]
- NASA, through Marshall Space Flight Center under the Discovery Program Office
- Austrian Space Applications Programme (ASAP) of the Austrian Research Promotion Agency (FFG)
- Programme de Developement d'Experiences (PRODEX)
- French Space Agency (CNES)
- Swedish National Space Agency
- University of Bern, Switzerland
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In the observations of the BepiColombo mission, the previously unexplored southern inner magnetosphere of Mercury was discovered, revealing different ion populations and signs of erosion in the magnetosphere. This is crucial for understanding the behavior of Mercury's magnetosphere in such proximity to the Sun.
Mercury's southern innermagnetosphere is an unexplored region as it was not observed by earlier space missions. In October 2021, BepiColombomission has passed through this region during its firstMercury flyby. Here, we describe the observations of SERENA ion sensors nearby and inside Mercury's magnetosphere. An intermittent high-energy signal, possibly due to an interplanetary magnetic flux rope, has been observed downstream Mercury, together with low energy solar wind. Low energy ions, possibly due to satellite outgassing, were detected outside the magnetosphere. The dayside magnetopause and bow-shock crossing were much closer to the planet than expected, signature of a highly eroded magnetosphere. Different ion populations have been observed inside the magnetosphere, like low latitude boundary layer at magnetopause inbound and partial ring current at dawn close to the planet. These observations are important for understanding the weak magnetosphere behavior so close to the Sun, revealing details never reached before.
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