Centimeter and decimeter wavelength emissions from solar flares

Details Centimeter and decimeter wavelength emissions from solar flares Centimeter and decimeter wavelength emissions from solar flares

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006pnaoc...3..113w&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 3, No.

Astronomy and Astrophysics

Astronomy

Solar Flare, Radio Emission, Review, Emission Mechanism

Scientific paper

Centimeter and decimeter wavelength emissions are from energetic electrons that are believed to carry a significant fraction of the energy liberated during the impulsive phase of solar flares. Firstly the centimeter-wavelength source morphology and kinematics, the comparison of centimeter-wavelength and X-ray source properties, are reviewed in this article. Then some recent observation results of decimeter-wavelength emissions are introduced including type III bursts, fiber/zebra bursts, drifting pulsation structures (DPS), spikes and so on. The related emission mechanisms are also discussed.

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