Amplitude Dependence of Nonlinear Precipitation Blocking of Relativistic Electrons by Large Amplitude EMIC Waves.
EMIC
force bunching
nonlinear
precipitation blocking
radiation belts
wave‐particle interactions
Journal
Geophysical research letters
ISSN: 0094-8276
Titre abrégé: Geophys Res Lett
Pays: United States
ID NLM: 9882887
Informations de publication
Date de publication:
28 Jun 2022
28 Jun 2022
Historique:
received:
22
02
2022
revised:
06
06
2022
accepted:
07
06
2022
entrez:
17
10
2022
pubmed:
18
10
2022
medline:
18
10
2022
Statut:
ppublish
Résumé
Recent work has shown that ElectroMagnetic Ion Cyclotron (EMIC) waves tend to occur in four distinct regions, each having their own characteristics and morphology. Here, we use nonlinear test-particle simulations to examine the range of energetic electron scattering responses to two EMIC wave groups that occur at low L-shells and overlap the outer radiation belt electrons. The first group consists of low-density, H-band region b waves, and the second group consists of high-density, He-band region c waves. Results show that while low-density EMIC waves cannot precipitate electrons below ∼16 MeV, the high density EMIC waves drive a range of linear and nonlinear behaviors including phase bunching and trapping. In particular, a nonlinear force bunching effect can rapidly advect electrons at low pitch-angles near the minimum resonant energy to larger pitch angles, effectively blocking precipitation and loss. This effect contradicts conventional expectations and may have profound implication for observational campaigns.
Identifiants
pubmed: 36246783
doi: 10.1029/2022GL098365
pii: GRL64375
pmc: PMC9541690
doi:
Types de publication
Journal Article
Langues
eng
Pagination
e2022GL098365Informations de copyright
© 2022. The Authors.
Déclaration de conflit d'intérêts
The authors declare no conflicts of interest relevant to this study.
Références
Nat Commun. 2016 Sep 28;7:12883
pubmed: 27678050