【摘 要】
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This paper provides a broad observation-based overview of the physical nature of the solar wind plasma and the embedded heliospheric magnetic field. Emphasis is on the spatial and temporal structure o
【机 构】
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Laboratory for Atmospheric and Space Physics University of Colorado
【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
This paper provides a broad observation-based overview of the physical nature of the solar wind plasma and the embedded heliospheric magnetic field. Emphasis is on the spatial and temporal structure of the wind, the relation of that structure to structure in the solar corona, and the evolution of the wind with heliocentric distance, including the nature of the winds interaction with the interstellar medium in the outermost regions of the solar system. The overview will also include discussion of suprathermal particles, current sheets, turbulence, magnetic topology, magnetic reconnection, and minor solar wind constituents.
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