Generation of Resonance Transition Emissions in the Solar Atmosphere

Details Generation of Resonance Transition Emissions in the Solar Atmosphere Generation of Resonance Transition Emissions in the Solar Atmosphere

Apr 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001astl...27..254f&link_type=abstract

Astronomy Letters, vol. 27, p. 254-259 (2001)

Astronomy and Astrophysics

Astronomy

12

Solar Flares, Small-Scale Turbulence, Plasma Diagnostics

Scientific paper

We derive formulas for the radio flux generated in solar flares by the resonance transition mechanism. This mechanism is shown to produce the observed decimeter-wave emission in continuum radio bursts at a level of small-scale irregularities of 10^{-6} - 10^{-7}. Thus, an analysis of continuum decimeter emission offers a unique opportunity to study small-scale turbulence in solar flares.

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