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Classification of New Spectral Lines of Fe XVII Observed in Solar Active Regions

Published online by Cambridge University Press:  14 August 2015

R. J. Hutcheon
R. J. Hutcheon*
Affiliation:
Dept. of Physics, University of Leicester, England

Summary

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This summary reports new emission lines of Fe XVII observed in two coronal active regions (McMath regions 12624, 12628). The lines were recorded by a Bragg plane crystal spectrometer collimated to 3′ FWHM, with a gypsum crystal scanning the wavelength range 8–14 Å. This spectrometer, part of a three spectrometer package previously used by Parkinson (1972, 1973), was mounted aboard a Skylark rocket (SL 1206) launched from Woomera at 0535 UT on 26th November 1973. One of the active regions studied (12624) was observed about 60 minutes 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. 69 - 70
Copyright
Copyright © Reidel 1975 

References

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