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Characteristics of the interplanetary shocks formed by a sudden increase in the velocity of the solar wind from a coronal hole (1995)

Bravo, S.

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Publication Date: 2011-08-24

Description: Coronal holes are the sources of the solar wind and, according to recent YOKOH observations, may undergo rapid changes which are associated with manifestations of explosive solar activity. Rapid changes in a hole's structure will produce rapid changes in the characteristics of the wind emerging from it and, in the particular c se of a sudden increase in wind velocity, this may lead to the formation of an interplanetary shock. We discuss the characteristics of shocks formed in such a way and compare them with interplanetary observations.

Keywords: Solar Physics

Type: International Solar Wind 8 Conference; 99; NASA-CR-199940

Format: text

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