Observations of solar active regions and solar flares by OSO-7

Details Observations of solar active regions and solar flares by OSO-7 Observations of solar active regions and solar flares by OSO-7

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977stin...7816977n&link_type=abstract

Presented at the OSO Workshop, Boulder, Colo., 8 Nov. 1977

Physics

Oso-7, Solar Activity, Solar Corona, Solar Flares, Photosphere, Solar Magnetic Field, Spectroheliographs, Sunspots, Ultraviolet Radiation

Scientific paper

Contributions made to the physics of coronal active regions and flares by the extreme ultraviolet and soft X-ray spectroheliograph on OSO-7 were discussed. Coronal structures above active regions were discussed from the point of view of their morphology and physical properties, including their relationship to photospheric and coronal magnetic fields. OSO-7 also recorded flares with sufficient spatial and temporal resolution to record, in some instances for the first time, the extreme ultraviolet and soft X-ray emission associated with such chromospheric phenomena as filament activation and the emergence of satellite sunspots. Flare phenomena were reviewed in terms of the several stages of evolution typically associated with the event.

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