CORDIS Project
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This project develops a global plasma simulation model to study Mercury's interaction with solar wind. It focuses on understanding the unique space weather processes at Mercury, utilizing advanced computing to analyze the planet's magnetosphere and exosphere.
We develop a new type of a global plasma simulation model with adaptive charged particle kinetic physics for the Mercury-solar wind interaction.
Mercury’s solar wind interaction, or space weather, is unique in the solar system due to spatially small and temporally fast magnetospheric scales, airless solid body with a large conducting core, a tenuous surface-originating exosphere and the closest distance to the Sun of the planets.
These features mean that Mercury is an ideal ""compact-sized magne…
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