The energy spectra of solar flare hydrogen, helium, oxygen, and iron - Evidence for stochastic acceleration

Details The energy spectra of solar flare hydrogen, helium, oxygen, and iron - Evidence for stochastic acceleration The energy spectra of solar flare hydrogen, helium, oxygen, and iron - Evidence for stochastic acceleration

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...401..398m&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 401, no. 1, p. 398-410.

Astronomy and Astrophysics

Astrophysics

42

Energy Spectra, Solar Flares, Solar Spectra, Spectral Energy Distribution, Abundance, Helium, Hydrogen, Iron, Oxygen, Particle Acceleration

Scientific paper

The time-integrated differential energy spectra of H, He, O, and Fe measured in 10 large flare events observed at 1 AU over the energy range of 0.3-80 MeV/nucleon showed consistent patterns in their spectral shapes: particles with larger mean mass-to-charge ratios were generally less abundant at higher energies. A steady state model of stochastic particle acceleration with rigidity-dependent diffusion coefficients fit the spectra best; spectra representative of diffusive shock acceleration also described the spectra of some events with the same number of free parameters, but often fell off faster in energy above 30 MeV per nucleon than the observations. The two model predictions differed most at energies near 0.1 MeV per nucleon, below the lowest energies observed in this study. The stochastic model quantitatively described the observed spectral ordering with less efficient acceleration of species with larger mean mass-to-charge ratios.

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