Energetic electron precipitation driven by electromagnetic ion cyclotron waves from ELFIN's low altitude perspective
Creators: name: Angelopoulos, V.
name: Zhang, X. -J.
name: Artemyev, A. V.
name: Mourenas, D.
name: Tsai, E.
name: Wilkins, C.
name: Runov, A.
name: Liu, J.
name: Turner, D. L.
name: Li, W.
name: Khurana, K.
name: Wirz, R. E.
name: Sergeev, V. A.
name: Meng, X.
name: Wu, J.
name: Hartinger, M. D.
name: Raita, T.
name: Shen, Y.
name: An, X.
name: Shi, X.
name: Bashir, M. F.
name: Shen, X.
name: Gan, L.
name: Qin, M.
name: Capannolo, L.
name: Ma, Q.
name: Russell, C. L.
name: Masongsong, E. V.
name: Caron, R.
name: He, I.
name: Iglesias, L.
name: Jha, S.
name: King, J.
name: Kumar, S.
name: Le, K.
name: Mao, J.
name: McDermott, A.
name: Nguyen, K.
name: Norris, A.
name: Palla, A.
name: Roosnovo
name: Tam, J.
name: Xie, E.
name: Yap, R. C.
name: Ye, S.
name: Young, C.
name: Adair, L. A.
name: Shaffer, C.
name: Chung, M.
name: Cruce, P.
name: Lawson, M.
name: Leneman, D.
name: Allen, M.
name: Anderson, M.
name: Arreola-Zamora, M.
name: Artinger, J.
name: Asher, J.
name: Branchevsky, D.
name: Cliffe, M.
name: Colton, K.
name: Costello, C.
name: Depe, D.
name: Domae, B. W.
name: Eldin, S.
name: Fitzgibbon, L.
name: Flemming, A.
name: Frederick, D. M.
name: Gilbert, A.
name: Hesford, B.
name: Krieger, R.
name: Lian, K.
name: McKinney, E.
name: Miller, J. P.
name: Pedersen, C.
name: Qu, Z.
name: Rozario, R.
name: Rubly, M.
name: Seaton, R.
name: Subramanian, A.
name: Sundin, S. R.
name: Tan, A.
name: Thomlinson, D.
name: Turner, W.
name: Wing, G.
name: Wong, C.
name: Zarifian, A.
Publisher: name: arXiv
Year: 2022
Subjects: subject: Space Physics (physics.space-ph)
subject: Plasma Physics (physics.plasm-ph)
subject: FOS: Physical sciences
subject: FOS: Physical sciences

description: We review comprehensive observations of electromagnetic ion cyclotron (EMIC) wave-driven energetic electron precipitation using data from the energetic electron detector on the Electron Losses and Fields InvestigatioN (ELFIN) mission, two polar-orbiting low-altitude spinning CubeSats, measuring 50-5000 keV electrons with good pitch-angle and energy resolution. EMIC wave-driven precipitation exhibits a distinct signature in energy-spectrograms of the precipitating-to-trapped flux ratio: peaks at 0.5 MeV which are abrupt (bursty) with significant substructure (occasionally down to sub-second timescale). Multiple ELFIN passes over the same MLT sector allow us to study the spatial and temporal evolution of the EMIC wave - electron interaction region. Using two years of ELFIN data, we assemble a statistical database of 50 events of strong EMIC wave-driven precipitation. Most reside at L=5-7 at dusk, while a smaller subset exists at L=8-12 at post-midnight. The energies of the peak-precipitation ratio and of the half-peak precipitation ratio (our proxy for the minimum resonance energy) exhibit an L-shell dependence in good agreement with theoretical estimates based on prior statistical observations of EMIC wave power spectra. The precipitation ratio's spectral shape for the most intense events has an exponential falloff away from the peak (i.e., on either side of 1.45 MeV). It too agrees well with quasi-linear diffusion theory based on prior statistics of wave spectra. Sub-MeV electron precipitation observed concurrently with strong EMIC wave-driven 1MeV precipitation has a spectral shape that is consistent with efficient pitch-angle scattering down to 200-300 keV by much less intense higher frequency EMIC waves. These results confirm the critical role of EMIC waves in driving relativistic electron losses. Nonlinear effects may abound and require further investigation.