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Particle energization in space plasmas: towards a multi-point, multi-scale plasma observatory

Retino Alessandro; Khotyaintsev Yuri; Le Contel Olivier; Marcucci Maria Federica; Plaschke Ferdinand; Vaivads Andris; Angelopoulos Vassilis; Blasi Pasquale; Burch Jim; De Keyser Johan; Dunlop Malcolm; Dai Lei; Eastwood Jonathan; Fu Huishan; Haaland Stein; Hoshino Masahiro; Johlander Andreas; Kepko Larry; Kucharek Harald; Lapenta Gianni; Lavraud Benoit; Malandraki Olga; Matthaeus William; McWilliams Kathryn; Petrukovich Anatoli; Pincon Jean-Louis; Saito Yoshifumi; Sorriso-Valvo Luca; Vainio Rami; Wimmer-Schweingruber Robert

Particle energization in space plasmas: towards a multi-point, multi-scale plasma observatory

Retino Alessandro
Khotyaintsev Yuri
Le Contel Olivier
Marcucci Maria Federica
Plaschke Ferdinand
Vaivads Andris
Angelopoulos Vassilis
Blasi Pasquale
Burch Jim
De Keyser Johan
Dunlop Malcolm
Dai Lei
Eastwood Jonathan
Fu Huishan
Haaland Stein
Hoshino Masahiro
Johlander Andreas
Kepko Larry
Kucharek Harald
Lapenta Gianni
Lavraud Benoit
Malandraki Olga
Matthaeus William
McWilliams Kathryn
Petrukovich Anatoli
Pincon Jean-Louis
Saito Yoshifumi
Sorriso-Valvo Luca
Vainio Rami
Wimmer-Schweingruber Robert
Katso/Avaa
Publisher´s pdf (2.784Mb)
Lataukset: 

SPRINGER
doi:10.1007/s10686-021-09797-7
URI
https://link.springer.com/article/10.1007%2Fs10686-021-09797-7
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Julkaisun pysyvä osoite on:
https://urn.fi/URN:NBN:fi-fe2022012710679
Tiivistelmä

This White Paper outlines the importance of addressing the fundamental science theme "How are charged particles energized in space plasmas" through a future ESA mission. The White Paper presents five compelling science questions related to particle energization by shocks, reconnection, waves and turbulence, jets and their combinations. Answering these questions requires resolving scale coupling, nonlinearity, and nonstationarity, which cannot be done with existing multi-point observations. In situ measurements from a multi-point, multi-scale L-class Plasma Observatory consisting of at least seven spacecraft covering fluid, ion, and electron scales are needed. The Plasma Observatory will enable a paradigm shift in our comprehension of particle energization and space plasma physics in general, with a very important impact on solar and astrophysical plasmas. It will be the next logical step following Cluster, THEMIS, and MMS for the very large and active European space plasmas community. Being one of the cornerstone missions of the future ESA Voyage 2050 science programme, it would further strengthen the European scientific and technical leadership in this important field.

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