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Impact of foreshock transients on near-Earth space

Project description

The impact of foreshock transients on near-Earth space dynamics

Collisionless shocks serve as powerful particle accelerators within astrophysical plasmas. Studies suggest that foreshock transients play a significant role in this acceleration process. These transients are particularly intriguing because they contribute to acceleration at the shock and have broader effects on geospace, generating rapid and intense wave storms within Earth's magnetosphere. The ERC-funded WAVESTORMS project has uncovered the capability of waves to accelerate energetic electrons within Earth’s radiation belts, thereby linking two key acceleration sites at Earth. Through a combination of multi-point in situ observations and global kinetic simulations, the project has untangled the intricate processes involved. The findings of this study promise to revolutionise our understanding of near-Earth space dynamics and particle acceleration in astrophysical contexts.

Objective

This project addresses major open questions in plasma physics: the dynamics of collisionless shocks, their impact on the downstream medium and particle acceleration. Collisionless shocks are powerful particle accelerators, ubiquitous in astrophysical plasmas. Recent works suggest that the dynamics of the shock precursor, or foreshock, contributes greatly to shock acceleration. Here we use near-Earth space as a natural laboratory to quantify the impact of transient kinetic structures forming in the foreshock. These foreshock transients are particularly intriguing because in addition to contributing to acceleration at the shock itself, they impact geospace as a whole in driving swift, intense wave storms in Earth's magnetosphere. In this proposal, I present recent data revealing that these waves accelerate energetic electrons in Earth's radiation belts, connecting for the first time the dynamics of two major acceleration sites at Earth. This issue has never been explored because of considerable challenges: multi-point in situ observations and global kinetic simulations are needed to unravel the complex processes at work. The WAVESTORMS project makes full use of recent advances on both of these fronts to resolve the impact of foreshock transients on near-Earth space in a holistic manner. Using a flagship kinetic model of the global magnetosphere and high-fidelity space- and ground-based measurements, we will (1) fully characterise their interaction with the shock and their contribution to shock acceleration, (2) quantify the radiation belt response (acceleration and losses), (3) connect our findings to the solar wind context, to finally (4) quantify their global impact on near-Earth space. My expertise in foreshock physics and in combining multi-mission data and cutting-edge simulations puts me in a unique position to lead this project. Our results will constitute a breakthrough in our understanding of near-Earth space dynamics and particle acceleration in general.

Keywords

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Programme(s)

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Topic(s)

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Funding Scheme

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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

HELSINGIN YLIOPISTO
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.

€ 1 998 084,00
Address
FABIANINKATU 33
00014 HELSINGIN YLIOPISTO
Finland

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Activity type
Higher or Secondary Education Establishments
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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.

€ 1 998 084,00

Beneficiaries (1)

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