Transient Interplnetary Plasma Structures and Their Geo-effectiveness

Details Transient Interplnetary Plasma Structures and Their Geo-effectiveness Transient Interplnetary Plasma Structures and Their Geo-effectiveness

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsh21b1916s&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SH21B-1916

Physics

[1650] Global Change / Solar Variability, [2111] Interplanetary Physics / Ejecta, Driver Gases, And Magnetic Clouds, [2164] Interplanetary Physics / Solar Wind Plasma, [2784] Magnetospheric Physics / Solar Wind/Magnetosphere Interactions

Scientific paper

Previous studies have indicated the association of geomagnetic storms with various solar and interplanetary plasma features. In the present study two types of solar wind plasma structures namely, Magnetic cloud events (MCEs) and Bidirectional electron heat flux (BEHF) events have been taken to study the short-term changes and analyzed taking in to consideration their association with coronal holes, selecting these events occurred during solar maximum period. Analysis reveals distinctly different effects of these two signatures on geomagnetic field as well as on modulating the cosmic ray intensities. Magnetic cloud events are found more effective comparing to bidirectional events on short-term basis.

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