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Mercury in the solar wind: adaptive kinetic model for space weather at solar system's innermost planet

Project description

Solving Mercury’s space weather secrets

Mercury’s interaction with solar wind, termed space weather, presents unique challenges. With its small and fast magnetosphere, its airless surface, large conducting core, and close proximity to the Sun, Mercury serves as an ideal compact-sized magnetospheric solar wind interaction laboratory. The ERC-funded MEOW project addresses these challenges by developing an advanced global plasma simulation model featuring adaptive charged particle kinetic physics. This model, based on high-performance computing, will accurately simulate Mercury’s space weather processes and the interactions within its magnetosphere-exosphere system. The project aims to enhance our understanding of these processes through the BepiColombo mission’s observations, revealing new insights into space weather dynamics.

Objective

"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 magnetospheric solar wind interaction laboratory"" for spacecraft and model studies compared to Earth's much larger magnetosphere. Since Mercury's plasma environment is populated by a unique composition of exospheric heavy ions mixed with the solar wind, the magnetosphere is much smaller than at Earth and under stronger solar wind conditions, studying Mercury reveals new information on space weather processes in general. The main scientific objectives of the BepiColombo (BC) two-orbiter mission en-route to Mercury include the investigation of the structure and dynamics of the Hermean magnetosphere and exosphere. The new model to be developed in this project is based on high-performance computing and an adaptive algorithm for charged particle kinetic effects. This enables efficiently resolving Hermean space weather processes and the coupled, complex solar wind-magnetosphere-exosphere system at detail beyond current global models. The new model is applied in the interpretation of observations by BC with the focus on the role of charged particle effects in the physics of basic space weather processes."

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HORIZON-ERC - HORIZON ERC Grants

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Call for proposal

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(opens in new window) ERC-2023-COG

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Host institution

ILMATIETEEN LAITOS
Net EU contribution

Net EU financial contribution. The sum of money that the participant receives, deducted by the EU contribution to its linked third party. It considers the distribution of the EU financial contribution between direct beneficiaries of the project and other types of participants, like third-party participants.

€ 1 997 101,00
Address
Erik Palmenin aukio 1
00560 Helsinki
Finland

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Region
Manner-Suomi Helsinki-Uusimaa Helsinki-Uusimaa
Activity type
Research Organisations
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Total cost

The total costs incurred by this organisation to participate in the project, including direct and indirect costs. This amount is a subset of the overall project budget.

€ 1 997 101,00

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