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X-Ray Spectroscopy of Solar Active Regions During the Third Skylab Mission

Published online by Cambridge University Press:  14 August 2015

J. P. Pye ,
R. J. Hutcheon ,
J. H. Parkinson  and
K. A. Pounds
J. P. Pye
Affiliation:
Dept. of Physics, University of Leicester, England
R. J. Hutcheon
Affiliation:
Dept. of Physics, University of Leicester, England
J. H. Parkinson
Affiliation:
Dept. of Physics, University of Leicester, England
K. A. Pounds
Affiliation:
Dept. of Physics, University of Leicester, England

Summary

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This paper describes the analysis of soft X-ray spectra of solar active regions observed on a Skylark sounding rocket flight. The experiment was launched from Woomera, South Australia, at 0535 UT on 26th November 1973. The payload consisted of 3 plane scanning Bragg crystal spectrometers, covering the wavelength range 4 to 23 Å, and collimated to 3 arc min FWHM. The instrument was the same as that used by Parkinson (1972, 1973). The launch was part of a collaborative observing program with American Science & Engineering who obtained X-ray photographs of the Sun with the S0-54 ATM X-ray telescope, simultaneously with the Leicester observations. We report preliminary results for McMath region 12624 (S10 W28). This region was observed about 60 min after the peak of an importance – N, class CO flare.

Type
Part 2: Active Regions
Information
Symposium - International Astronomical Union , Volume 68: Solar X, Gamma, and EUV Radiation , 1975 , pp. 65 - 66
Copyright
Copyright © Reidel 1975 

References

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