The case for protons powering solar flares

Eos

Volumn 77, Issue 37, 1996, Pages

  Simnett, George M ^a  

^a UNIVERSITY OF BIRMINGHAM   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0038830885     PISSN: 00963941     EISSN: None     Source Type: Journal    
DOI: 10.1029/96EO00245     Document Type: Review

References (7)

1. Cliver, E. W., N. B. Crosby, and B. R. Dennis, Are solar gamma-ray-line flares different from other large flares?, Astrophys. J., 426, 767, 1994.
2. Ramaty, R., N. Mandzhavidze, B. Kozlovsky, and R. J. Murphy, Solar atmospheric abundances and energy content in flare-accelerated ions from gamma-ray spectroscopy, Astrophys J., 455, L193, 1995.
3. Sakao, T., Characteristics of solar flare hard X-ray sources, Ph.D. thesis, University of Tokyo, 1994.
4. Simnett, G. M., A dominant role for protons at the onset of solar flares, Sol. Phys., 106, 165, 1986.
5. Simnett, G. M., Protons in flares, Space Sci. Rev., 73, 387, 1995.
6. Simnelt, G. M., and M. G. Haines, On the production of hard X-rays in solar flares, Sol. Phys., 130, 253, 1990.
7. Simnett, G. M., and K. T. Strong, The impulsive phase of a solar limb flare, Astrophys. J., 284, 839, 1984.