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Primordial Flares, Flux Tubes, and Gamma-ray Bursts

Published online by Cambridge University Press:  25 May 2016

K. M. Hiremath
K. M. Hiremath*
Affiliation:
Indian Institute of Astrophysics, Bangalore-560034, India

Abstract

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Given the prevailing physical conditions in the cosmic environment, the similarity of solar transients and cosmic gamma-ray bursts suggests that the most promising energy source for the latter may be primordial flares, which derive energy from magnetic reconnection.

Type
Part II: Posters
Information
Symposium - International Astronomical Union , Volume 195: Highly Energetic Physical Processes and Mechanisms , 2000 , pp. 397 - 398
Copyright
Copyright © Astronomical Society of the Pacific 2000 

References

Gokhale, M. H., & Hiremath, K. M. 1986, Adv. Space Res., 6, no. 8, 47.CrossRefGoogle Scholar
Hood, A. W. 1986, in Solar System Magnetic Fields, ed. Priest, E. R. (Dordrecht: D. Reidel Publishing Company), 80.Google Scholar
Meegan, C., Hurley, A. C., Dingus, B., & Matz, S. 1997, in Proceedings of the IV Compton Symposium, eds. Dermer, C. D., Strickman, M. S., & Kurfess, J. D. (Woodbury: AIP), 407.Google Scholar
Parker, E. N. 1994, in Spontaneous Current Sheets in Magnetic Fields, ed. Parker, E. N. (Oxford: Oxford Univ. Press), 286.CrossRefGoogle Scholar
Priest, E. R. 1981, in Solar Flare Magnetohydrodynamics, ed. Priest, E. R. (New York: Gordon and Breach Science Publishers), 14.Google Scholar
Wentzel, D. G. 1977, Solar Phys., 52, 163.Google Scholar