Analysis of a Complex Solar Radio Burst

MA Yuan; WANG De-yu; WANG Min; YAN Yih-ua

Astronomical Research and Technology > 2009 > 6(2): 100-106.

MA Yuan, WANG De-yu, WANG Min, YAN Yih-ua. Analysis of a Complex Solar Radio Burst[J]. Astronomical Research and Technology, 2009, 6(2): 100-106.

Citation:

MA Yuan, WANG De-yu, WANG Min, YAN Yih-ua. Analysis of a Complex Solar Radio Burst[J]. Astronomical Research and Technology, 2009, 6(2): 100-106.

Citation:

MA Yuan, WANG De-yu, WANG Min, YAN Yih-ua. Analysis of a Complex Solar Radio Burst[J]. Astronomical Research and Technology, 2009, 6(2): 100-106.

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Analysis of a Complex Solar Radio Burst

1.
National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, China
2.
Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, China
3.
National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

More Information

Received Date: June 16, 2008
Revised Date: August 27, 2008
Published Date: April 14, 2009

Graphical Abstract

Abstract

Abstract

A complex solar radio burst observed with the spectrometers of NAOC working at 625~1500 MHz, 2600~3800MHz, and 5200~7600 MHz was analyzed in this paper.We probe the correlations of the radio data with the data of Hα flares, CME, and Hard X-rays of the same underlying burst, as well as those of related (terrestrial) atmospheric events.We have found some prominent features about the burst.We think that the electron-acceleration site may be in the outer corona——near the region corresponding to the frequency 625 MHz.We also think that the magnetic reconnection occurred several times, and the decay phase after the magnetic reconnection is a turbulence-acceleration process.
- Solar radio bursts,
- Hα flares,
- CME

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References (9)

References

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