Do protons or electrons dominate particle acceleration in solar flares?

Eos

Volumn 77, Issue 37, 1996, Pages 353-357

  Cargill, Peter ^a  

^a IMPERIAL COLLEGE LONDON   (United Kingdom)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0004878464     PISSN: 00963941     EISSN: None     Source Type: Journal    
DOI: 10.1029/96EO00242     Document Type: Review

References (8)

1. Anastasiadis, T., and L. Vlahos, Particle acceleration inside a gas of shock waves, Astron. Astrophys., 245, 271, 1991.
2. Benka, S. G., and G. D. Holman, A Thermal/nonthermal model for solar hard X-ray bursts, Astrophys. J., 435, 469, 1994.
3. Masuda, S., Hard X-ray sources and the primary energy release site in solar flares, Ph.D. thesis, University of Tokyo, 1994.
4. Miller, J. A., and D. A. Roberts, Stochastic proton acceleration by cascading Alfvén waves in impulsive solar flares, Astrophys. J., 452, 912, 1995.
5. Miller, J. A., T. N. Larosa, and R. L. Moore, Stochastic electron acceleration by cascading fast mode waves in impulsive solar flares, Astrophys. J., 461, 445, 1996.
6. 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.
7. Sakao, T., Characteristics of solar flare hard X-ray sources, Ph.D. thesis, University of Tokyo, 1994.
8. Winglee, R. M., G. A. Dulk, P. L. Bommann, and J. C. Brown, Interrelation of soft and hard X-ray emission during flares, II, Simulation model, Astrophys. J., 375, 382, 1991.