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Some Characteristics of the Development and Emissions of May 13, 1981 Flare Related to the Flare Model

Published online by Cambridge University Press:  12 April 2016

Ladislav Krivsky
Ladislav Krivsky*
Affiliation:
Astronomical Institute, Ondrejov 25165 Czechoslovakia

Abstract

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Proton flare of May 13, 1981 with various emissions and with registration of loop shaped flare in hard X-ray range above new created flare channel in Hα and Hβ is related with flare loop-model published earlier at IAU Symp. No. 35 in 1967.

Type
Session 6. Flares and Transients
Information
International Astronomical Union Colloquium , Volume 141: The Magnetic and Velocity Fields of Solar Active Regions , 1993 , pp. 359 - 361
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

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6. Takakura, T., Ohki, K., Tsuneta, S., Nitta, N., Makishima, K., Muraki, T., Ogawa, Y., Oda, N. 1982 in Hinotori Symp. on Solar Flares, Inst. of Space and Astronaut. Sci., Tokyo, 142 Google Scholar