【摘 要】
:
The typical differences in composition of the main components of different solar wind types are well-known.The good mass resolution of Mass-Time-Of-Flight(MTOF) on the Solar Helioshperic Observatory(S
【机 构】
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Christian-Albrechts-Universit at Kiel,Germany Uni
【出 处】
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The Fourteenth International Solar Wind Conference (第十四届国际太阳
论文部分内容阅读
The typical differences in composition of the main components of different solar wind types are well-known.The good mass resolution of Mass-Time-Of-Flight(MTOF) on the Solar Helioshperic Observatory(SOHO) allows us to investigate the composition of heavy minor elements in different types of solar wind as well.Based on the classification scheme taken from Xu and Borovsky [1] four types of solar wind plasma can be distinguished:coronal hole-origin,ejecta,streamer-origin and sectorreversalregion plasma.This classification scheme requires measurements of the magnet field.
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