Statistics of Multi‐MeV Electron Drift‐Periodic Flux Oscillations Using Van Allen Probes Observations
Statistics of Multi‐MeV Electron Drift‐Periodic Flux Oscillations Using Van Allen Probes Observations
复制标题
DOI:
10.1029/2022gl097995
复制
发表时间:
2022-03
影响因子:
5.2
通讯作者:
Hong Zhao;T. Sarris;Xinlin Li;Isabella G. Huckabee;D. Baker;A. Jaynes;S. Kanekal
中科院分区:
文献类型:
--
作者:
Hong Zhao;T. Sarris;Xinlin Li;Isabella G. Huckabee;D. Baker;A. Jaynes;S. Kanekal
Multi‐MeV electron drift‐periodic flux oscillations observed in Earth's radiation belts indicate radial transport and energization/de‐energization of these radiation belt core populations. Using multi‐year Van Allen Probes observations, a statistical analysis is conducted to understand the characteristics of this phenomenon. The results show that most of these flux oscillations result from resonant interactions with broadband ultralow frequency (ULF) waves and are indicators of ongoing radial diffusion. The occurrence frequency of flux oscillations is higher during high solar wind speed/dynamic pressure and geomagnetically active times; however, a large number of them were still observed under mild to moderate solar wind/geomagnetic conditions. The occurrence frequency is also highest (up to ∼30%) at low L‐shells ( L∗∼3−4 ${L}^{\ast }\sim 3-4$ ) under various geomagnetic activity, suggesting the general presence of broadband ULF waves and radial diffusion at low L‐shells even during geomagnetically quiet times and showing the critical role of the electron phase space density radial gradient in forming drift‐periodic flux oscillations.