Electron Acceleration in Solar Noise Storms

Details Electron Acceleration in Solar Noise Storms Electron Acceleration in Solar Noise Storms

Nov 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ihy..worke..39s&link_type=abstract

2nd UN/NASA Workshop on International Heliophysical Year and Basic Space Science. Proceedings of the conference held 27 Novembe

Astronomy and Astrophysics

Astrophysics

Scientific paper

We report high resolution, high dynamic range meter wavelength observations of noise storm sources in the solar corona. These observations were made by combining visibilities from the Giant Meterwave Radio Telescope (GMRT) in Pune, India, and the Nancay RadioHeliograph (NRH) in Nancay, France. These observations have the potential to place firm upper limits on the brightness temperature of noise storm sources. We have therefore carried out theoretical work on the energetics of non-thermal electron acceleration in noise storm sources. We have derived rigorous estimates for the overall efficiency of the overall noise storm emission process, beginning with non-thermal electron acceleration and culminating in the observed radiation.

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