The solar wind: A turbulent magnetohydrodynamic medium

被引:6
作者
Bavassano, B
机构
[1] Istituto di Fisica dello Spazio Interplanetario, Consiglio Nazionale delle Ricerche
[2] IFSI, CNR, 00044 Frascati, via G. Galilei
关键词
D O I
10.1007/BF00170789
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
MHD turbulence properties in the solar wind are briefly reviewed The evolution of fluctuations of alfvenic type in near-ecliptic regions of the inner heliosphere is described. The role of interplanetary sources and the influence of interactions with structures convected by the solar wind are discussed. Turbulence features at high latitudes and in the outermost regions of the heliosphere are finally highlighted.
引用
收藏
页码:29 / 32
页数:4
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