The distribution of maximum temperatures of coronal active region loops

Details The distribution of maximum temperatures of coronal active region loops The distribution of maximum temperatures of coronal active region loops

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a....93..228t&link_type=abstract

Astronomy and Astrophysics, vol. 93, no. 1-2, Jan. 1981, p. 228-234.

Astronomy and Astrophysics

Astronomy

Coronal Loops, Solar Activity, Solar Radiation, Solar Temperature, Temperature Distribution, Distribution Functions, Emission Spectra, Ultraviolet Astronomy, Weighting Functions, X Ray Astronomy

Scientific paper

Starting with the integrated emission measure distributions of solar active regions, the distribution of the maximum temperature parameter which characterizes individual plasma loops is determined. The observed emission measure distributions were determined by combining EUV and X-ray data from two separate experiments on ATM/Skylab. The present work sets some limits on such an approach. It is found that the distribution of maximum temperature has approximately the same shape as the integrated emission measure distributions, a result which is expected since most of the loop emission measure is near their maximum temperatures.

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