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Volume Characteristics of Magnetic-Channel Flares

Published online by Cambridge University Press:  14 August 2015

L. Křivský
L. Křivský*
Affiliation:
Astronomical Institute, Czechoslovak Academy of Sciences, Ondřejov, Czechoslovakia

Abstract

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On the basis of Hα pictures of two proton flares of medium size, the volume of the separate parts of magnetic-channel flares, are given. At the time of the main release of energy the volume of the whole system is determined at ∼ 2.5 × 1027 cm3 and the size of areas III after Petschek model at ∼ 7.0 × 1020 cm3.

Type
Part IV: Observations of Magnetic Fields Associated with Flares and Other Transitory Phenomena
Information
Symposium - International Astronomical Union , Volume 43: Solar Magnetic Fields , 1971 , pp. 443 - 449
Copyright
Copyright © Reidel 1971 

References

Acton, L. W.: 1968, Astrophys. J. 152, 305.Google Scholar
Bruzek, A. and DeMastus, H. L.: 1970, Solar Phys. 12, 447.Google Scholar
De Jager, C.: 1967, in Electromagnetic Radiation in Space , (ed. by Emming, J. G.), D. Reidel Publ. Co., Dordrecht-Holland, p. 101.Google Scholar
De Jager, C.: 1969, in Öhman, Y. (ed.), ‘Mass Motions in Solar Flares and Related Phenomena’, Nobel Symp. 9, 171.Google Scholar
Ellison, M., McKenna, S. M. P., and Reid, J. H.: 1961, Dunsink Observ. Publ. 1, 53.Google Scholar
Friedman, M. and Hamberger, S. M.: 1969, Solar Phys. 8, 104.Google Scholar
Křivský, L.: 1963, Bull. Astron. Inst. Czech. 14, 77.Google Scholar
Křivský, L.: 1968, in Kiepenheuer, K. O. (ed.), ‘Structure and Development of Solar Active Regions’, IAU Symp. 35, 465.Google Scholar
Křivský, L.: 1969a, Bull. Astron. Inst. Czech. 20, 139.Google Scholar
Křivský, L.: 1969b, Bull. Astron. Inst. Czech. 20, 163.Google Scholar
Křivský, L.: 1970, Bull. Astron. Inst. Czech. 21, 67.Google Scholar
Křivský, L.: and Švestka, Z.: 1970, Space Research X , COSPAR XII, Prague 1969 (ed. Donahue, et al.), North-Holland, Amsterdam, p. 817.Google Scholar
Neupert, W. M.: 1969, Ann. Rev. Astron. Astrophys. 7, 121.CrossRefGoogle Scholar
Petschek, H. E.: 1964, in AAS-NASA Symp. Physics of Solar Flares 1963 , Washington, p. 425.Google Scholar
Švestka, Z.: 1966, Space Sci. Rev. 5, 388.Google Scholar
Švestka, Z.: 1970, Solar Phys. 13, 471.Google Scholar
Takakura, T.: 1969, Solar Phys. 6, 133.CrossRefGoogle Scholar
Vaiana, G. S., Reidy, W. P., Zehnpfennig, T., Van Speybroeck, L., and Giacconi, R.: 1968, Science 161, 564.Google Scholar
Vaiana, G. S. and Giacconi, R.: 1969, in Plasma Instabilities in Astrophysics , (ed. by Wentzel, and Tidman, ), Gordon and Breach, New York, p. 91.Google Scholar
Valníček, B.: 1967, Bull. Astron. Inst. Czech. 18, 249.Google Scholar
Zirin, H.: 1964, Astrophys. J. 140, 1216.Google Scholar