Interplanetary Transient Solar Wind Plasma Flows and Their Influence on the Geomagnetic Activities (P25)

Details Interplanetary Transient Solar Wind Plasma Flows and Their Influence on the Geomagnetic Activities (P25) Interplanetary Transient Solar Wind Plasma Flows and Their Influence on the Geomagnetic Activities (P25)

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ihy..worke.117k&link_type=abstract

2nd UN/NASA Workshop on International Heliophysical Year and Basic Space Science. Proceedings of the conference held 27 Novembe

Astronomy and Astrophysics

Astrophysics

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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