ORIGIN AND EVOLUTION OF MHD TURBULENCE IN THE SOLAR-WIND

被引：3

作者：

BAVASSANO, B

机构：

[1] Istituto di Fisica dello Spazio Interplanetario, C.N.R., Frascati (Roma), 00044

来源：

NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA C-GEOPHYSICS AND SPACE PHYSICS | 1990年 / 13卷 / 01期

关键词：

Interplanetary space;

D O I：

10.1007/BF02515777

中图分类号：

学科分类号：

摘要：

Solar wind turbulence has both solar and interplanetary sources. Outward travelling waves are generated at the Sun with a spectrum related to the turbulent processes in the solar atmosphere. Instabilities at velocity shears give a local contribution of waves with inward and outward propagation. Nonlinear interactions between the two kinds of waves lead to an energy cascade and to a Kolmogoroff spectrum. © 1990 Società Italiana di Fisica.

引用

页码：79 / 87

页数：9

共 18 条

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