Transient phenomena in the solar atmosphere and solar wind

Details Transient phenomena in the solar atmosphere and solar wind Transient phenomena in the solar atmosphere and solar wind

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976tpsa.book.....g&link_type=abstract

Presented at the Intern. Symp. on Solar Terrestrial Phys., Boulder, Colo., 7-18 Jun. 1976

Physics

1

Interplanetary Magnetic Fields, Magnetic Disturbances, Solar Activity, Solar Atmosphere, Solar Wind, Coronagraphs, Gas Dynamics, Solar Corona, Stellar Mass Ejection

Scientific paper

Observations of transient disturbances in the solar atmosphere are reviewed with emphasis on two classes of coronal mass ejection events. Large flare associated events travel more than twice as fast (on the average) as the prominence associated events. Mass and energy content of the two classes may also differ, because flare associated events are massive and energetic and produce shock wave disturbances at 1 AU. The slower moving prominence events do not.

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