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基于范艾伦卫星观测数据的地球辐射带电子能谱分布的统计分析

王建行 项正 马新 郭德宇 董俊虎 刘阳希子 胡景乐 倪彬彬

空间科学学报2024,Vol.44Issue(3):446-457,12.
空间科学学报2024,Vol.44Issue(3):446-457,12.DOI:10.11728/cjss2024.03.2023-0070

基于范艾伦卫星观测数据的地球辐射带电子能谱分布的统计分析

Statistical Analysis of Distributions of Electron Energy Spectra in the Earth's Radiation Belts Based on Van Allen Probes Observations

王建行 1项正 1马新 1郭德宇 1董俊虎 1刘阳希子 1胡景乐 1倪彬彬1

作者信息

  • 1. 武汉大学空间物理系 武汉 430072
  • 折叠

摘要

Abstract

The characteristics of energy spectra distributions of radiation belt electrons can help re-veal the dominant physical mechanism behind the dynamics of the radiation belt.In this study,the tem-poral and spatial distribution characteristics of energy spectra of energetic electrons are statistically ana-lyzed using the measurements from Van Allen probes during 2014-2018.The results show that most of the electron spectra in the radiation belt can be classified into three types:exponential,power-law and reversed spectra.The exponential spectra dominate in the outer radiation belt outside the plasmapause.The power-law spectra usually occur at higher L values and move to lower L values during geomagnetic storms.During quiet geomagnetic activity periods,the power-law energy spectra stay at the high L with longer time and higher proportion.The reversed energy spectra dominate at L>2.5 inside the plasmas-phere.As the increase of plasmapause locations,more reversed energy spectra occur while the propor-tion of the exponential energy spectra decreases.During long-term quiet periods,electron fluxes near the peak of the reversed energy spectra(about 2 MeV)are relatively low to form obvious reversed spectral.The results also show that the peak location of reversed energy spectra is about 2 L inside the plasma-pause while the peak location of exponential energy spectra is about 1.5 L outside the plasmapause.Ap-pearances of power-law energy spectra are related to substorm injections of electrons.Stronger magnetic storms produce wider L ranges where reversed energy spectra are replaced by exponential spectra.Dur-ing quiet times,exponential energy spectra inside the plasmapause are replaced by reversed energy spec-tra due to pitch angle scattering produced by plasmaspheric hiss waves.

关键词

辐射带/电子能谱/范艾伦探测器/地磁活动/等离子体层层顶

Key words

Radiation belts/Electron energy spectra/Van Allen Probes/Geomagnetic activity/Plasmapause

分类

天文与地球科学

引用本文复制引用

王建行,项正,马新,郭德宇,董俊虎,刘阳希子,胡景乐,倪彬彬..基于范艾伦卫星观测数据的地球辐射带电子能谱分布的统计分析[J].空间科学学报,2024,44(3):446-457,12.

基金项目

国家自然科学基金项目(42025404,42188101,42174190),国家重点研发计划基金项目(2022YFF0503700),中国科学院战略性先导科技专项(B类)(XDB41000000)和民用航天技术预先研究项目(D020308,D020104)共同资助 (42025404,42188101,42174190)

空间科学学报

OA北大核心CSTPCD

0254-6124

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