Turkish Journal of Physics
DOI
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Abstract
Activity has many manifestations, from dark spots to bright regions, to the presence of the heated chromosphere, to the superheated corona. Sunspots are extended, strongly magnetic regions on the Sun. Photospheric faculae are generally visible only at the limb. Polar faculae are smaller than the main-zone faculae. The contributions of the active region faculae and the facular network are at least as important as the solar spots in augmenting the solar emission.
First Page
383
Last Page
390
Recommended Citation
EVREN, SERDAR (1999) "Facular Structures on Cool Stars," Turkish Journal of Physics: Vol. 23: No. 2, Article 10. Available at: https://journals.tubitak.gov.tr/physics/vol23/iss2/10
