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Kinetic Investigation of Simulated Magnetosheath Electron Trajectories and Spacecraft Potential Accumulation RisK

Project description

Studying satellite surface charging during geosynchronous magnetopause crossings

The number of satellites has increased in recent years, making them vital for everyday life and communication. However, satellites face challenges in space, particularly from the build-up of charged particles, mainly fast-moving electrons. This accumulation can cause sudden electrical discharges, potentially leading to damage or total loss of the spacecraft. Supported by the Marie Skłodowska-Curie Actions programme, the KISMET-SPARK project will conduct the first dedicated study of surface charging during geosynchronous magnetopause crossing (GMC) events. During GMCs, the solar wind compresses the Earth’s magnetic field, placing satellites in geosynchronous orbit within the magnetosheath region, where intense surface charging and elevated electron fluxes can occur. The study aims to improve understanding of space weather and help develop more resilient satellite systems.

Objective

"Satellites in space are subjected to charged particles in the ambient environment. Specifically, the fast-moving electrons of the space plasma can rapidly accumulate on satellite surfaces. These surfaces may then suddenly discharge in electrical arcs that damage the onboard electronics, which may even result in total loss of the spacecraft. The project KISMET-SPARK will be the first dedicated study of surface charging during rare but impactful events known as ""Geosynchronous Magnetopause Crossings"" (GMCs). During a GMC, the solar wind compresses the Earth's magnetic field. This ends up placing satellites in Geosynchronous Earth Orbit (GEO) within a region known as the magnetosheath, where the ambient electron fluxes and resulting surface charging can be intense.

In KISMET-SPARK, the Applicant Konstantinos Horaites will address the kinetic physics of electrons in Earth's magnetosheath and their space weather impacts. In two Work Packages, he will 1) describe the processes that shape the energized ""flat-top"" electron velocity distribution (eVDF), and 2) evaluate how these electrons contribute to the costly GEO satellite failures that are correlated with GMCs. The project will be supervised by Daniel Verscharen, who is an Associate Professor at the Host institution, the University of College London's Mullard Space Science Laboratory. The Applicant will simulate the magnetosheath environment using state-of-the-art kinetic ""eVlasiator"" simulations of Earth's magnetosheath. He will employ the Supervisor's ""ALPS"" code to assess the kinetic stability of the eVDF, which will explain the origin of the flat-top population. This project will combine the Applicant's experience with simulations together with the Supervisor's knowledge of space-plasma instabilities, to answer long-standing questions about the magnetosheath eVDF's origins and impacts. The project results will be communicated to the scientific community, industry stakeholders, and the general public."

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HORIZON-TMA-MSCA-PF-EF - HORIZON TMA MSCA Postdoctoral Fellowships - European Fellowships

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(opens in new window) HORIZON-MSCA-2024-PF-01

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Coordinator

UNIVERSITY COLLEGE LONDON
Net EU contribution

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€ 260 347,92
Address
GOWER STREET
WC1E 6BT LONDON
United Kingdom

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Region
London Inner London — West Camden and City of London
Activity type
Higher or Secondary Education Establishments
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Total cost

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