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- W2171497415 abstract "We review recent progress in the possible role of micro turbulence in the solar wind. The solar wind is expected to excite plasma microinstabilities owing to its transition from a collision-dominated to a collisionless plasma, with potentially drastic consequences for thermal transport and other physical processes. We discuss both the extensive linear theory of this subject and also our present understanding of nonlinear plasma turbulence. The solar wind is an excellent laboratory for studying many aspects of solar and plasma physics, and may soon provide some answers to several fundamental questions." @default.
- W2171497415 created "2016-06-24" @default.
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- W2171497415 date "1980-07-29" @default.
- W2171497415 modified "2023-09-27" @default.
- W2171497415 title "Instabilities in the solar wind" @default.
- W2171497415 doi "https://doi.org/10.1098/rsta.1980.0231" @default.
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