A Broadband Radiospectrometer and Fine Structures in Microwave Bursts

Details A Broadband Radiospectrometer and Fine Structures in Microwave Bursts A Broadband Radiospectrometer and Fine Structures in Microwave Bursts

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999spro.proc..433f&link_type=abstract

Solar Physics with Radio Observations, Proceedings of the Nobeyama Symposium, held in Kiyosato, Japan, Oct. 27-30, 1998, Edited

Physics

1

Scientific paper

Since 1994, a project for setting up a solar radio broadband spectrograph with high resolution in time and frequency has been carried out. Some new and interesting results obtained with 2.6--3.8 GHz and 1.0--2.0 GHz radio spectrometers are briefly introduced. This equipment will be the key observation facility in coming solar maximum years in China.

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