Origin and Early Evolution of Coronal Mass Ejections

Details Origin and Early Evolution of Coronal Mass Ejections Origin and Early Evolution of Coronal Mass Ejections

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agusm..sh61a01g&link_type=abstract

American Geophysical Union, Spring Meeting 2001, abstract #SH61A-01 INVITED

Physics

7513 Coronal Mass Ejections, 7531 Prominence Eruptions, 7534 Radio Emissions, 7851 Shock Waves

Scientific paper

Simultaneous observations at multiple wavelengths over a large field of view have dramatically improved our understanding of coronal mass ejections. Extreme ultraviolet and soft X-ray observations reveal the source regions of Earth-directed CMEs. Microwave and H-alpha observations provide information on the cool components of the CMEs. Radio observations at long decametric and hectometric wavelengths trace CME-driven shock waves that just enter into the interplanetary medium. This paper summarizes recent findings on CMEs using SOHO, Yohkoh and Wind observations and discusses how near-Sun CME observations are useful in interpreting transient events in the inner heliosphere.

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