An investigation of the relationship between the magnetic storm Dst-index and different types of solar wind streams

Details An investigation of the relationship between the magnetic storm Dst-index and different types of solar wind streams An investigation of the relationship between the magnetic storm Dst-index and different types of solar wind streams

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993angeo..11..678e&link_type=abstract

Annales Geophysicae (ISSN 0992-7689), vol. 11, no. 8, p. 678-684.

Physics

8

Interplanetary Magnetic Fields, Magnetic Storms, Solar Terrestrial Interactions, Solar Wind, Current Sheets, Heliosphere, Indexes (Ratios)

Scientific paper

In this paper it is shown that the intensity of the negative Bz-component of the IMF in the region of interaction of fast and slow quasi-stationary solar wind streams can be the source of rather strong magnetic storms with Dst less than 100 nT. It is found that the level of magnetic disturbance, caused by sporadic solar wind streams, depends largely on characteristics of the medium through which these streams propagate.

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