Fine Structures Observed by the Chinese Solar Radio Broadband Fast Dynamic Spectrometers

Details Fine Structures Observed by the Chinese Solar Radio Broadband Fast Dynamic Spectrometers Fine Structures Observed by the Chinese Solar Radio Broadband Fast Dynamic Spectrometers

May 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003aspc..289..401y&link_type=abstract

The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume I, held 2-5 July 2002 at National Center of Sciences, Hito

Astronomy and Astrophysics

Astronomy

Scientific paper

Observations by the newly established Chinese Solar Radio Broadband Fast Dynamic Spectrometers (Fu et al. 1995) in the 0.7--7.6 GHz frequency range are introduced. The instrument has been working properly in the 23rd solar maximum with very high temporal (5, 8, 100 ms) and spectral (1.4, 10, 20 MHz) resolutions simultaneously. The observational results are helpful for a better understanding of particle acceleration and energy conversion in the solar corona.

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