Solar Radio Bursts on 16 February 1999 |
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Authors: | Zongjun Ning Qijun Fu Yihua Yan Yuying Liu Quankang Lu |
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Institution: | (1) Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing, 100012, China;(2) National Astronomical Observatory, Chinese Academy of Sciences, Beijing, 100012, China;(3) Department of Physics, University of Fudan, Shanghai, 200433, China |
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Abstract: | The 2.60–3.80 GHz spectrometer at the Beijing Astronomical Observatory (BAO) recorded a ‘decimetric pulsation’ event (DCIM)
around the time 1999 0216 0300. At the beginning and end of this DCIM, two groups of reverse slope type III bursts (RS-III)
are also detected; meanwhile, metric type II bursts are recorded by CULG and HIRA during the same time. These solar radio
bursts on that day might be caused by the same active region 8458 and a same flare. We present a plausible qualitative model
for all of them.
This revised version was published online in July 2006 with corrections to the Cover Date. |
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