Closed loop model of turbulent acceleration for the gradual phase of the radio burst of 1981 April 27

Details Closed loop model of turbulent acceleration for the gradual phase of the radio burst of 1981 April 27 Closed loop model of turbulent acceleration for the gradual phase of the radio burst of 1981 April 27

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acasn..32..186y&link_type=abstract

(Acta Astronomica Sinica, vol. 32, no. 2, 1991, p. 186-193) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 15, Dec. 1

Astronomy and Astrophysics

Astrophysics

Particle Acceleration, Plasma Turbulence, Solar Flares, Solar Radio Bursts, Gamma Ray Bursts, Solar X-Rays, Stochastic Processes

Scientific paper

A closed-loop model of turbulent stochastic acceleration is proposed for
the gradual phase of the radio burst of April 27, 1981. It can explain
the various observed features in the spectrum, the rather long time of
rise, the absence of X-ray bursts below 56 keV, and of any detectable
proton events.

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