The Coronal Emission Spectrum
نویسندگان
چکیده
منابع مشابه
Coronal emission and dynamo saturation
We show that the observed saturation of X-ray emission with increasing rotation rate in solar-type stars does not necessarily imply saturation of the underlying dynamo. This effect can be caused by the centrifugal stripping of the corona. As the stellar rotation rate is increased, centrifugal forces cause a rise in the pressure and density in the outer parts of the largest magnetic loops. This ...
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ژورنال
عنوان ژورنال: Monthly Notices of the Royal Astronomical Society
سال: 1948
ISSN: 0035-8711,1365-2966
DOI: 10.1093/mnras/108.3.292