Relationship between substorm activity and the interplanetary medium parameters during the main phase of strong magnetic storms

Author:

Boroyev R.N.

Funder

Russian Foundation for Basic Research – Russia

Publisher

Elsevier BV

Subject

Space and Planetary Science,Aerospace Engineering,General Earth and Planetary Sciences,Atmospheric Science,Geophysics,Astronomy and Astrophysics

Reference23 articles.

1. Auroral substorms and the interplanetary magnetic field;Akasofu;J. Geophys. Res.,1973

2. Measurement and Analysis of Random Data;Bendat,1971

3. Differences between CME driven storms and CIR driven storms;Borovsky;J. Geophys. Res.,2006

4. Magnetic field at geosynchronous orbit during highspeed stream-driven storms: connections to the solar wind, the plasma sheet, and the outer electron radiation belt;Borovsky;J. Geophys. Res.,2010

5. Correlation between auroral activity and rate of development of a storm in its main phase;Boroyev;Solar-Terrestrial Phys.,2016

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