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What are the fundamental modes of energy transfer and partitioning in the coupled Magnetosphere-Ionosphere system?

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posted on 2023-01-12, 16:55 authored by Jonathan Rae, Colin Forsyth, Malcolm Dunlop, Minna Palmroth, Mark Lester, Reiner Friedel, Geoff Reeves, Larry Kepko, Lucille Turc, Clare Watt, Wojciech Hajdas, Theodoros Sarris, Yoshifumi Saito, Ondrej Santolik, Yuri Shprits, Chi Wang, Aurelie Marchaudon, Matthieu Berthomier, Octav Marghitu, Benoit Hubert, Martin Volwerk, Elena A Kronberg, Ian Mann, Kyle Murphy, David Miles, Zhonghua Yao, Andrew Fazakerley, Jasmine Sandhu, Hayley Allison, Quanqi Shi
The fundamental processes responsible for energy exchange between large-scale electromagnetic fields and plasma are well understood theoretically, but in practice these theories have not been tested. These processes are ubiquitous in all plasmas, especially at the interface between high and low beta plasmas in planetary magnetospheres and other magnetic environments. Although such boundaries pervade the plasma Universe, the processes responsible for the release of the stored magnetic and thermal plasma energy have not been fully identified and the importance of the relative impact of each process is unknown. Despite advances in understanding energy release through the conversion of magnetic to kinetic energy in magnetic reconnection, how the extreme pressures in the regions between stretched and more relaxed field lines in the transition region are balanced and released through adiabatic convection of plasma and fields is still a mystery. Recent theoretical advances and the predictions of large-scale instabilities must be tested. In essence, the processes responsible remain poorly understood and the problem unresolved. The aim of the White Paper submitted to ESA’s Voyage 2050 call, and the contents of this paper, is to highlight three outstanding open science questions that are of clear international interest: (i) the interplay of local and global plasma physics processes: (ii) the partitioning during energy conversion between electromagnetic and plasma energy: and (iii) what processes drive the coupling between low and high beta plasmas. We present a discussion of the new measurements and technological advances required from current state-of-the-art, and several candidate mission profiles with which these international high-priority science goals could be significantly advanced.

Funding

I. J. Rae is supported by STFC grant ST/S000240/1, and NERC grants NE/P017150/1, NE/ P017185/1, NE/V002724/1 and NE/V002554/1. M. W. Dunlop is supported by an STFC in-house research grant ST/M001083/1, a NERC grant NE/P016863/1 and the NSFC grants 41574155 and 41431071. C. Watt is supported by STFC grant ST/R000921/1. E. A. Kronberg is supported by a German Research Foundation (DFG) grant KR 4375/2-1 within SPP “Dynamic Earth”. O. Marghitu acknowledges support by ESA contracts 4000127660 MAGICS and 4000118383 SIFACIT. D. Miles is supported by faculty startup funding from the University of Iowa

History

Citation

Rae, J., Forsyth, C., Dunlop, M. et al. What are the fundamental modes of energy transfer and partitioning in the coupled Magnetosphere-Ionosphere system?. Exp Astron (2022). https://doi.org/10.1007/s10686-022-09861-w

Author affiliation

School of Physics and Astronomy

Version

VoR (Version of Record)

Published in

EXPERIMENTAL ASTRONOMY

Pagination

(36)

Publisher

SPRINGER

issn

0922-6435

eissn

1572-9508

Acceptance date

2022-07-09

Copyright date

2022

Available date

2023-01-12

Language

English