A comparison of outer electron radiation belt dropouts during solar wind stream interface and magnetic cloud driven storms

被引:0
作者
O Ogunjobi
V Sivakumar
Z Mtumela
机构
[1] North–West University,Center for Space Research, School for Physical and Chemical Sciences
[2] University of KwaZulu-Natal,School of Chemistry and Physics
来源
Journal of Earth System Science | 2017年 / 126卷
关键词
Stream interfaces; magnetic clouds; magnetosphere; Earth’s radiation belts; L-shell;
D O I
暂无
中图分类号
学科分类号
摘要
Energetic electrons are trapped in the Earth’s radiation belts which occupy a toroidal region between 3 and 7 RE\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\hbox {R}_{\mathrm{E}}$$\end{document} above the Earth’s surface. Rapid loss of electrons from the radiation belts is known as dropouts. The source and loss mechanisms regulating the radiation belts population are not yet understood entirely, particularly during geomagnetic storm times. Nevertheless, the dominant loss mechanism may require an event based study to be better observed. Utilizing multiple data sources from the year 1997–2007, this study identifies radiation belt electron dropouts which are ultimately triggered when solar wind stream interfaces (SI) arrived at Earth, or when magnetic clouds (MC) arrived. Using superposed epoch analysis (SEA) technique, a synthesis of multiple observations is performed to reveal loss mechanism which might, perhaps, be a major contributor to radiation belt losses under SI and MC driven storms. Results show an abrupt slower decaying precipitation of electron peak (about 3000 counts/sec) on SI arrival within 5.05 <L\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$< L$$\end{document} < 6.05, which persist till 0.5 day before gradual recovery. This pattern is interpreted as an indication of depleted electrons from bounce lost cone via precipitating mechanism known as relativistic electron microburst. On the other hand, MC shows a pancake precipitating peak extending to lower L (Plasmapause); indicating a combination of electron cyclotron harmonic (ECH) and whistler mode waves as the contributing mechanisms.
引用
收藏
相关论文
共 15 条
  • [1] A comparison of outer electron radiation belt dropouts during solar wind stream interface and magnetic cloud driven storms
    Ogunjobi, O.
    Sivakumar, V.
    Mtumela, Z.
    JOURNAL OF EARTH SYSTEM SCIENCE, 2017, 126 (04)
  • [2] Dropouts of the outer electron radiation belt in response to solar wind stream interfaces: global positioning system observations
    Morley, Steven K.
    Friedel, Reiner H. W.
    Spanswick, Emma L.
    Reeves, Geoffrey D.
    Steinberg, John T.
    Koller, Josef
    Cayton, Thomas
    Noveroske, Evan
    PROCEEDINGS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, 2010, 466 (2123): : 3329 - 3350
  • [3] Determination of Outer Radiation Belt MeV Electron Energization Rates and Delayed Response Times to Solar Wind Driving During Geomagnetic Storms
    Srinivas, P.
    Spencer, E.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2024, 129 (07)
  • [4] On the influence of solar wind conditions on the outer-electron radiation belt
    Kellerman, A. C.
    Shprits, Y. Y.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2012, 117
  • [5] ELECTRON RADIATION BELT DYNAMICS DURING MAGNETIC STORMS AND IN QUIET TIME
    Lazutin, L. L.
    Dmitriev, A. V.
    Suvorova, A. V.
    SOLAR-TERRESTRIAL PHYSICS, 2018, 4 (01): : 51 - 60
  • [6] Characterizing magnetopause shadowing effects in the outer electron radiation belt during geomagnetic storms
    Herrera, D.
    Maget, V. F.
    Sicard-Piet, A.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2016, 121 (10) : 9517 - 9530
  • [7] On the problem of electron loss in the outer radiation belt during a magnetic storm
    Lazutin, L. L.
    GEOMAGNETISM AND AERONOMY, 2016, 56 (05) : 545 - 556
  • [8] Significant loss of energetic electrons at the heart of the outer radiation belt during weak magnetic storms
    Hwang, J.
    Lee, D-Y.
    Kim, K-C.
    Shin, D-K.
    Kim, J-H.
    Cho, J-H.
    Park, M-Y.
    Turner, D. L.
    JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 2013, 118 (07) : 4221 - 4236
  • [9] Dynamic variations of the outer radiation belt during magnetic storms for 1.5-6.0 MeV electrons
    Yuan ChongJing
    Zong QiuGang
    SCIENCE CHINA-TECHNOLOGICAL SCIENCES, 2011, 54 (02) : 431 - 440
  • [10] Radiation belt electron flux variability during three CIR-driven geomagnetic storms
    Lam, M. M.
    Horne, R. B.
    Meredith, N. P.
    Glauert, S. A.
    JOURNAL OF ATMOSPHERIC AND SOLAR-TERRESTRIAL PHYSICS, 2009, 71 (10-11) : 1145 - 1156