Solar flares, magnetic clouds, and geomagnetic storms

Details Solar flares, magnetic clouds, and geomagnetic storms Solar flares, magnetic clouds, and geomagnetic storms

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..143..365i&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 143, no. 2, p. 365-372.

Physics

4

Earth Ionosphere, Environment Effects, Experiment Design, Ionospheric Disturbances, Spaceborne Experiments, Environmental Monitoring, Mathematical Models, Rocket Launching, Short Wave Radio Transmission

Scientific paper

Firstly, semiempirical distributions of solar wind proton number density and velocity ordered around the Heliospherical Current Sheet (HCS) of the inner heliosphere are considered. Then, the velocity profiles of flare-generated Coronal Mass Ejections running through the inhomogeneous heliosphere are calculated. They show that the velocities strongly depend on flare positions with respect to the HCS. Finally, a specific mutual flare-HCS-earth location leading to a strong geomagnetic storm is deduced from calculations and supported by a few real events of solar-terrestrial physics.

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