A three-component concept of the chromosphere and transition region

Details A three-component concept of the chromosphere and transition region A three-component concept of the chromosphere and transition region

Aug 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974soph...37..317f&link_type=abstract

Solar Physics, vol. 37, Aug. 1974, p. 317-321.

Physics

4

Chromosphere, Faculae, Optical Transition, Solar Granulation, Solar Temperature, Far Ultraviolet Radiation, Microwave Emission, Solar Atmosphere, Temperature Distribution

Scientific paper

It is proposed that present observations of the chromosphere and transition region in EUV, optical and mm wavelengths are best described by a three-component concept. The three components are taken to be the interiors of supergranular cells, the hot plagettes overlying faculae, and the cooler, transient mottles which surround them in the network boundaries. The enhanced emission of the hot plagettes in transition ions is interpreted as a direct result of the increased pressure scale height over faculae relative to the cell interiors.

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