MICROWAVE SOLAR RADIO EVENTS

LIU Yuying; FU Qijun; NING Zongjun

doi:10.11728/cjss2002.01.20020101

Volume 22 Issue 1

Feb. 2002

Turn off MathJax

Article Contents

Article Navigation > Chinese Journal of Space Science > 2002 > 22(1): 1-5

LIU Yuying, FU Qijun, NING Zongjun. MICROWAVE SOLAR RADIO EVENTS[J]. Chinese Journal of Space Science, 2002, 22(1): 1-5. doi: 10.11728/cjss2002.01.20020101

Citation:

LIU Yuying, FU Qijun, NING Zongjun. MICROWAVE SOLAR RADIO EVENTS[J]. Chinese Journal of Space Science, 2002, 22(1): 1-5. doi: 10.11728/cjss2002.01.20020101

LIU Yuying, FU Qijun, NING Zongjun. MICROWAVE SOLAR RADIO EVENTS[J]. Chinese Journal of Space Science, 2002, 22(1): 1-5. doi: 10.11728/cjss2002.01.20020101

Citation:

LIU Yuying, FU Qijun, NING Zongjun. MICROWAVE SOLAR RADIO EVENTS[J]. Chinese Journal of Space Science, 2002, 22(1): 1-5. doi: 10.11728/cjss2002.01.20020101

PDF( 451 KB)

MICROWAVE SOLAR RADIO EVENTS

doi: 10.11728/cjss2002.01.20020101 cstr: 32142.14.cjss2002.01.20020101

National Astronomical Observatories. The Chinese Academy of Sciences, Beijing 100012

Received Date: 2001-03-02
Rev Recd Date: 2001-08-10

Abstract

Abstract

The two solar radio spectrometers on the bands of 1.0-2.0GHz and 2.63.8 GHz respectively have put into operation at National Astronomical Observatory of China （NAOC） from January 1994 and September 1996. There have been 297 and 316 solar radio events recorded up to April 10, 2000 by these two spectrometers. High sensitivity as well as high frequency and time resolution is characterized by these records. They provide a rich and valuable information for studying the evolution process of solar flare with the various time periods. A typical solar radio event of them on April l5, 1998 shows a variety of the morphological features and fine structures on this frequency range.
- Spectrometers,
- Observation,
- Solar radio events