On magnetic field stochasticity and nonthermal line broadening in solar flares

Details On magnetic field stochasticity and nonthermal line broadening in solar flares On magnetic field stochasticity and nonthermal line broadening in solar flares

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...301..975a&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 301, Feb. 15, 1986, p. 975-980. CNR-supported research.

Astronomy and Astrophysics

Astrophysics

24

Solar Flares, Solar Magnetic Field, Solar Spectra, Spectral Line Width, Stochastic Processes, Magnetic Field Reconnection, Particle Acceleration, Plasma Equilibrium, Plasma Spectra, Solar Maximum Mission, Turbulent Flow, X Ray Spectra

Scientific paper

Observations of nonthermal line broadening seen in solar flares by the Solar Maximum Mission satellite are discussed in light of recent results on the generation of magnetic field stochasticity. It is shown that a consistent model for the data can be constructed by assuming that the observations signal the destruction of an ambient magnetohydrodynamic equilibrium.

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