Characteristics of gamma-ray line flares
β
Taeil Bai; B. R. Dennis; A. L. Kiplinger; L. E. Orwig; K. J. Frost
π
Article
π
1983
π
Springer
π
English
β 572 KB
Observations of gamma-ray lines from solar flares by SMM demonstrated that energetic protons and heavy ions are accelerated during the impulsive phase. In order to understand the acceleration mechanism for gamma-ray producing protons and heavy ions, we have studied the characteristics of the flares