New Perspective on Phase Space Density Analysis for Outer Radiation Belt Enhancements: The Influence of MeV Electron Injections

被引:8
作者
Kim, H. -J. [1 ]
Kim, K. -C. [2 ]
Noh, S. -J. [3 ]
Lyons, L. [1 ]
Lee, D. -Y. [2 ]
Choe, W. [4 ]
机构
[1] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA 90095 USA
[2] Chungbuk Natl Univ, Dept Astron & Space Sci, Cheongju, South Korea
[3] Los Alamos Natl Lab, Los Alamos, NM USA
[4] May & June Solut, Seoul, South Korea
基金
新加坡国家研究基金会;
关键词
relativistic electron enhancements; radiation belts; injections; MeV electrons; substorm; rapid electron enhancements; RELATIVISTIC ELECTRONS; ACCELERATION; STORM;
D O I
10.1029/2023GL104614
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
Observation of growing phase space density (PSD) peak in the outer electron radiation belt has been considered evidence for local wave-driven acceleration as a primary cause of radiation belt enhancement. However, recent studies showed that strong substorm-associated MeV electron injections can also cause significant radiation belt enhancements on fast timescales (& SIM;10s min). Such rapid enhancements pose challenges for determining true spatial PSD profiles. To address this, we conduct a detailed spatiotemporal analysis of electron flux and PSD during an enhancement event, using Van Allen Probes data. Our analysis reveals rapid and intermittent flux enhancements. During these rapid enhancements, inbound spacecraft observed false PSD peaks, due to spacecraft's relatively slow movement. However, we identify time intervals of stable fluxes between enhancements, enabling us to determine quasi-stationary PSD profiles with no noticeable peaks. This study provides new insights into accurate PSD analysis, critical for understanding the mechanisms underlying radiation belt enhancements.
引用
收藏
页数:10
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