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On the correlation between chromospheric and coronal emissionIt is shown that with increasing stellar activity the emission of the transition region and corona increases faster than the emission of the chromosphere. It is also explained why the pressure of the transition region increases with increasing stellar activity. Further, it is shown that this relation is a necessary requirement for the global stability of the chromosphere/transition region/corona system.
Document ID
19820023326
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Hammer, R. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Linsky, J. L. (Joint Inst. for Lab. Astrophysics Boulder, CO, United States)
Endler, F. (Wuerzburg Univ.)
Date Acquired
August 10, 2013
Publication Date
January 1, 1982
Publication Information
Publication: NASA. Goddard Space Flight Center Advan. in Ultraviolet Astron.
Subject Category
Astronomy
Accession Number
82N31202
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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