A possible mechanism of nonresonant heating of the chromosphere-corona transition zone

Details A possible mechanism of nonresonant heating of the chromosphere-corona transition zone A possible mechanism of nonresonant heating of the chromosphere-corona transition zone

Sep 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979acasn..20..281l&link_type=abstract

Acta Astronomica Sinica, vol. 20, Sept. 1979, p. 281-288. In Chinese, with abstract in English.

Astronomy and Astrophysics

Astronomy

3

Chromosphere, Plasma Heating, Plasma Oscillations, Solar Corona, Energetic Particles, Plasma-Particle Interactions, Proton Beams, Temperature Distribution

Scientific paper

An attempt is made to explain the steep vertical temperature distribution in the solar chromosphere-corona transition region on the basis of a mechanism involving pileup of plasma oscillations and wave-particle nonresonant heating. Analysis shows that if a high-energy proton beam is continuously injected into the transition region from the chromosphere, the steep temperature distribution arises in a narrow layer through nonlinear wave-particle interactions.

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