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.
The Proceedings of the IAU 8th Asian-Pacific Regional Meeting, Volume 1
- Pub Date:
- May 2003