Properties of Large Angle CMEs and Their Space Weather Effects (P23)

Details Properties of Large Angle CMEs and Their Space Weather Effects (P23) Properties of Large Angle CMEs and Their Space Weather Effects (P23)

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ihy..worke.115j&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

Using IPS observations, CMEs (Coronal Mass Ejections) have been detected over the entire Sun-Earth distance (Manoharan et al. 1995). The effects of large CMEs (angular width >1500) are studied and reported here. The effects of such CMEs on the interplanetary medium (IPM) are sensed by the Interplanetary Scintillation (IPS) recorded at Rajkot and at Ooty. The Radio Telescope detects the signatures of Interplanetary Disturbances resulting either from CME or CIR (Co-rotating Interaction Region). The solar observations of these CME and associated events are presented. We also discuss the space weather aspects of CMEs.

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