TY - JOUR
T1 - Resonant Whistler-Electron Interactions
T2 - MMS Observations Versus Test-Particle Simulation
AU - Behar, E.
AU - Sahraoui, F.
AU - Berčič, L.
N1 - Publisher Copyright:
©2020. American Geophysical Union. All Rights Reserved.
PY - 2020/10/1
Y1 - 2020/10/1
N2 - We present a novel technique to analyze VDF, which allows to capture their fine structure including wave-particles resonances. By applying the technique to magnetospheric multiscale (MMS) data, the simultaneous observation of characteristic three-dimensional (3-D) signatures in the electron velocity distribution function (VDF) and intense quasi-monochromatic waves in the terrestrial magnetosheath is investigated. The intense wave packets are characterized and modeled analytically as quasi-parallel circularly polarized whistler waves and applied to a test-particle simulation in view of gaining insight into the signature of the wave-particle resonances in velocity space. Both the Landau and the cyclotron resonances were evidenced in the test-particle simulations. The location and general shape of the test-particle signatures do account for the observations, but the finer details, such as the symmetry of the observed signatures, are not matched, indicating either the limits of the test-particle approach or a more fundamental physical mechanism not yet grasped. Finally, it is shown that the energization of the electrons in this precise resonance case cannot be diagnosed using the moments of the distribution function, as done with the classical E · J “dissipation” estimate.
AB - We present a novel technique to analyze VDF, which allows to capture their fine structure including wave-particles resonances. By applying the technique to magnetospheric multiscale (MMS) data, the simultaneous observation of characteristic three-dimensional (3-D) signatures in the electron velocity distribution function (VDF) and intense quasi-monochromatic waves in the terrestrial magnetosheath is investigated. The intense wave packets are characterized and modeled analytically as quasi-parallel circularly polarized whistler waves and applied to a test-particle simulation in view of gaining insight into the signature of the wave-particle resonances in velocity space. Both the Landau and the cyclotron resonances were evidenced in the test-particle simulations. The location and general shape of the test-particle signatures do account for the observations, but the finer details, such as the symmetry of the observed signatures, are not matched, indicating either the limits of the test-particle approach or a more fundamental physical mechanism not yet grasped. Finally, it is shown that the energization of the electrons in this precise resonance case cannot be diagnosed using the moments of the distribution function, as done with the classical E · J “dissipation” estimate.
KW - MMS observations
KW - magnetosheath
KW - test-particles
KW - wave-particle resonance
KW - whistler mode wave
U2 - 10.1029/2020JA028040
DO - 10.1029/2020JA028040
M3 - Article
AN - SCOPUS:85093960801
SN - 2169-9402
VL - 125
JO - Journal of Geophysical Research: Space Physics
JF - Journal of Geophysical Research: Space Physics
IS - 10
M1 - e2020JA028040
ER -