Nonlinear resonant interaction of radiation belt electrons with intense whistler-mode waves
journal contribution
posted on 2025-01-29, 16:54authored byA Artemyev, D Mourenas, X-J Zhang, O Agapitov, Anatoly NeishtadtAnatoly Neishtadt, D Vainchtein, A Vasiliev, X Zhang, Q Ma, I Bortnik, V Krasnoselskikh
<p dir="ltr">The dynamics of the Earth’s outer radiation belt, filled by energetic electron fluxes, is largely controlled by electron resonant interactions with electromagnetic whistler-mode waves. The most coherent and intense waves resonantly interact with electrons nonlinearly, and the observable effects of such nonlinear interactions cannot be described within the frame of classical quasi-linear models.</p><p dir="ltr">This paper provides an overview of the current stage of the theory of nonlinear resonant interactions and discusses different possible approaches for incorporating these nonlinear interactions into global radiation belt simulations. We focus on observational properties of whistler-mode waves and theoretical aspects of nonlinear resonant interactions between such waves and energetic electrons. We consider only sufficiently energetic particles, which can be treated as test particles and do not have a significant feedback to the waves. The review covers two main regimes of nonlinear resonant wave-particle interactions: the regime of long wave-packets, historically better studied, and the regime of short wave-packets, actively investigated more recently based on refined spacecraft observations.</p>
Funding
NASA contracts 80NSSC20K0218, 80NSSC22K0433, 80NSSC22K0522, 80NSSC20K0697, and 80NSSC21K1770
NASA grants 80NSSC20K0196 and 80NSSC24K0572
NSF grant AGS-2225445
NASA 80NSSC22K1637, NASA/HTMS 80NSSC20K1270 subcontract through Boston University
NSF/GEM award 2225613
NSF/GEM award AGS- 2025706
CNES ”Solar Orbiter” and ”Parker Solar Probe” projects
NASA contract 80NSSC21K1770
NASA contracts 80NSSC24K0138, 80NSSC23K0100, 80NSSC23K0108, 80NSSC22K0522, 80NSSC23K1038, 80NSSC24K0561, 80NSSC19K0844
This version of the article has been accepted for publication, after peer review (when applicable) and is subject to Springer Nature’s AM terms of use, but is not the Version of Record and does not reflect post-acceptance improvements, or any corrections. The Version of Record is available online at: http://dx.doi.org/[insert DOI]