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Solar wind halo/strahl electron populations carry important information on the formation of suprathermal electrons in the solar wind.
Solar Wind~0.1-2 keV Electrons at Quiet Times
【摘 要】
：
Solar wind halo/strahl electron populations carry important information on the formation of suprathermal electrons in the solar wind.
【作 者】
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【机 构】
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School of Earth and Space Science,Peking University,Beijing 100871,China
【出 处】
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The Fourteenth International Solar Wind Conference (第十四届国际太阳
【发表日期】
：
2015年5期
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