Physical Characteristics of Coronal Region Driving Out the Interplanetary Shock

Details Physical Characteristics of Coronal Region Driving Out the Interplanetary Shock Physical Characteristics of Coronal Region Driving Out the Interplanetary Shock

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008jass...25...25o&link_type=abstract

Journal of Astronomy and Space Sciences. Vol. 25, no. 1, 025-032

Astronomy and Astrophysics

Astronomy

Ace, Interplanetary Shock, Icme

Scientific paper

Using the solar wind data of 2000 observed by ACE, We classified the interplanetary shock on basis of shock driver. We examined the physical properties of shock drivers such as the ratio of charge states(O7/O6) and thermal index(I_{th}). Most of 51 interplanetary shocks are driven by interplanetary coronal mass ejections(ICME; magnetic cloud and ejecta) and high speed streams. According to the test of temperature(O7/O6) and I_{th}, we found that ICMEs originated from region with hot source in corona.

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