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太阳风中的Alfven波耗散与电子和质子温度分布问题
引用本文:肖池阶,宋礼庭.太阳风中的Alfven波耗散与电子和质子温度分布问题[J].空间科学学报,1998,18(4):296-300.
作者姓名:肖池阶  宋礼庭
作者单位:北京大学地球物理系!100871
基金项目:国家自然科学基金!49774249
摘    要:根据动力论Alfven波耗散机制,详细计算了动力论Alfven波衰减的能量分配给质子和电子的比率.初步解释了高速太阳风中质子温度比电子温度高的事实,定性说明了r<10Rs时电子快速冷却的原因.

关 键 词:动力论Alfven波  高速太阳风  质子温度  电子温度

THE TEMPERATURE DISTRIBUTION BETWEEN PROTONS AND ELECTRONS AND THE DISSIPATION OF KINETIC ALFVEN WAVES IN THE SOLAR WIND
XIAO Chijie, SONG Liting.THE TEMPERATURE DISTRIBUTION BETWEEN PROTONS AND ELECTRONS AND THE DISSIPATION OF KINETIC ALFVEN WAVES IN THE SOLAR WIND[J].Chinese Journal of Space Science,1998,18(4):296-300.
Authors:XIAO Chijie  SONG Liting
Abstract:The dissipation energy ratio of kinetic Alfven waves between proton and electrons is calculated in details based on the dissipation principle of kinetic Alfven waves. It provides a simple explanation of the fact of the higher proton temperature compared with electrons in high speed stream of the solar wind. The rapid cooling of electrons at r<10Rs is explained qualitatively.
Keywords:Kinetic Alfven wave  High-speed stream of solar wind  Tempeature of proton  Temperature of electron
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