Solar gamma-ray lines as probes of accelerated particle directionalities in flares

Details Solar gamma-ray lines as probes of accelerated particle directionalities in flares Solar gamma-ray lines as probes of accelerated particle directionalities in flares

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975sgla.book.....r&link_type=abstract

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Physics

Gamma Rays, Line Spectra, Particle Acceleration, Solar Flares, Angular Distribution, Charged Particles, Doppler Effect, Energy Distribution, Monte Carlo Method

Scientific paper

Anisotropies of charged particles accelerated in solar flares were studied by observing Doppler shifts of selected gamma-ray lines. The spectral shape was calculated of the 6.1-MeV line of O-16. If the accelerated particles are isotropic, the line remains centered at e0 = 6129.4 keV, and its width (FWHM) is about 100 keV. For particle anisotropies that may be produced in solar flares, the line is shifted to lower energies by about 30 to 40 keV.

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