【摘 要】
：
High speed streams are often characterized by a core proton temperature anisotropy such that Tp⊥＞Tp‖ and by a minority population of alpha particles such that(v)α‖＞(v)p‖,where(v)‖ is the component of
【机 构】
：
Space Science 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
High speed streams are often characterized by a core proton temperature anisotropy such that Tp⊥＞Tp‖ and by a minority population of alpha particles such that(v)α‖＞(v)p‖,where(v)‖ is the component of the bulk velocity parallel to the mean magnetic field defined so that(v)s‖＞0 when the parallel component of the flow velocity is directed awayfrom the sun.
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