Transient Solar Wind Plasma Flows and their Influence on the Geomagnetic Activity

Details Transient Solar Wind Plasma Flows and their Influence on the Geomagnetic Activity Transient Solar Wind Plasma Flows and their Influence on the Geomagnetic Activity

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd...3e..90k&link_type=abstract

Solar Active Regions and 3D Magnetic Structure, 26th meeting of the IAU, Joint Discussion 3, 16-17 August, 2006, Prague, Czech R

Computer Science

Scientific paper

Geomagnetic storms are well known to be associated with solar and interplanetary magnetic activities. In the present study, we consider two types of solar wind plasma flow phenomena, namely, magnetic cloud events and bidirectional electron heat flux events and discuss their short-term changes and analyze their association with coronal holes. We select those events that took place during solar maximum. Analysis reveals distinctly different effects of these two signatures on geomagnetic field. Magnetic cloud events are found more effective comparing to bidirectional events on short-term basis.

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