Formation of the 0.511 MeV line in solar flares

• 1 December 1976
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 210, 582-592
• https://doi.org/10.1086/154863

Abstract

Keywords

• GAMMA RAYS
• POSITRON ANNIHILATION
• POSITRONIUM
• SOLAR FLARES
• SOLAR X-RAYS
• SPECTRAL LINE WIDTH
• CONTINUOUS SPECTRA
• COULOMB COLLISIONS
• DISTRIBUTION FUNCTIONS
• ENERGY DISTRIBUTION
• FREE ELECTRONS
• MONTE CARLO METHOD
• RADIATIVE RECOMBINATION
• SOLAR ATMOSPHERE
• TEMPERATURE EFFECTS