【摘 要】
：
Near the Sun(＜～10Rs) the acceleration,heating,and propagation of the solar wind is likely affected by the background inhomogeneities of the magnetized plasma.
【机 构】
：
CUA/NASA GSFC Weizmann Institute
【出 处】
：
The Fourteenth International Solar Wind Conference (第十四届国际太阳
论文部分内容阅读
Near the Sun(＜～10Rs) the acceleration,heating,and propagation of the solar wind is likely affected by the background inhomogeneities of the magnetized plasma.
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