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Solar X-Ray Source Unassociated with Sunspots

Published online by Cambridge University Press:  12 April 2016

G. A. Gurzadyan
Affiliation:
Space Research Branch of Byurakan Astrophysical Observatory, Erevan, Armenian S.S.R., U.S.S.R.
K. V. Vartanian
Affiliation:
Space Research Branch of Byurakan Astrophysical Observatory, Erevan, Armenian S.S.R., U.S.S.R.

Extract

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On October 3, 1970 the astrophysical rocket observatory K-2 was launched from the Soviet Union, designed to investigate the Sun in the region of short- and X-ray waves Gurzadyan et al. (1971). During the launching a series of X-ray pictures of the Sun was received, in the period 04 h 22 min to 04 h 30 min universal time, through an aluminum foil 5000 Å thick, covering a polistriol film 1000 Å thick. The pictures were taken by means of a pinhole camera under the following conditions: the focal length was 150 mm, the angular resolution – from 8’ to 0.’92, which corresponds to the dimensions of the input diaphragm from 0.28 mm to 0.04 mm, effective exposure – 520s, the pointing accuracy by a stabilised platform carrying the instruments – 0.′7-0.′8. The picture was taken by a film of the UF-R type (Kalinkina et al, 1965).

Type
Section IV / The Solar Soft X-Ray Spectrum
Copyright
Copyright © Reidel 1972

References

Gurzadyan, G. A., Kazarian, E. A., Krmoyan, M. N., and Epremian, R. A.: 1971, Doklady Akad. Nauk Arm. S.S.R. 53, 224.Google Scholar
Kalinkina, T. A., Oshurkova, A. N., Pankova, A. A., Uvarova, V. M., Tshistova, G. I., and Shpolskij, M. R.: 1965, J. Priclad. Spectrosc. 2, 475.Google Scholar
Soln. Dann. 1970, Bull. No. 10, October, Leningrad.Google Scholar