The Source of Multi Spectral Energy of Solar Energetic Electron

被引:0
|
作者
Herdiwijaya, Dhani [1 ,2 ]
机构
[1] Intitute Technol Bandung, Fac Math & Nat Sci, Astron Div, Bandung 40132, Indonesia
[2] Intitute Technol Bandung, Fac Math & Nat Sci, Bosscha Observ, Bandung 40132, Indonesia
来源
关键词
energetic electron; flare; coronal mass ejection; coronal hole;
D O I
10.1063/1.4917154
中图分类号
O59 [应用物理学];
学科分类号
摘要
We study the solar energetic electron distribution obtained from ACE and GOES satellites which have different altitudes and electron spectral energy during the year 1997 to 2011. The electron spectral energies were 0.038-0.315 MeV from EPAM instrument onboard ACE satellite and >2 MeV from GOES satellite. We found that the low electron energy has no correlation with high energy. In spite of we have corrected to the altitude differences. It implied that they originated from time dependent events with different sources and physical processes at the solar atmosphere. The sources of multi spectral energetic electron were related to flare and CME phenomena. However, we also found that high energetic electron comes from coronal hole.
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页数:3
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