Statistical Analyses of the Type Ⅲ Bursts and CMEs During the 23rd Solar Cycle

MA Yuan; WANG De-yu; YAN Yi-hua

Astronomical Research and Technology > 2006 > 3(4): 321-327.

MA Yuan, WANG De-yu, YAN Yi-hua. Statistical Analyses of the Type Ⅲ Bursts and CMEs During the 23rd Solar Cycle[J]. Astronomical Research and Technology, 2006, 3(4): 321-327.

Citation:

MA Yuan, WANG De-yu, YAN Yi-hua. Statistical Analyses of the Type Ⅲ Bursts and CMEs During the 23rd Solar Cycle[J]. Astronomical Research and Technology, 2006, 3(4): 321-327.

Citation:

MA Yuan, WANG De-yu, YAN Yi-hua. Statistical Analyses of the Type Ⅲ Bursts and CMEs During the 23rd Solar Cycle[J]. Astronomical Research and Technology, 2006, 3(4): 321-327.

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Statistical Analyses of the Type Ⅲ Bursts and CMEs During the 23rd Solar Cycle

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

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Received Date: January 24, 2006
Revised Date: March 21, 2006
Published Date: October 14, 2006

Graphical Abstract

Abstract

Abstract

The Statistics analyses of the microwave type Ⅲ bursts,coronal mass ejections(CMEs),Hαflares and relevant events observed with 5200-7600MHz spectrograph at the National Astronomical Observatory during the 23^rd solar cycle are carried out in this article.It is found that the relation between the microwave type Ⅲ bursts and CMEs is not closer than that between the type Ⅱ radio bursts and CMEs;the Hαflares corresponding to the CMEs are all gradual flares.
- Microwave type Ⅲ bursts,
- Hαflares,
- CMEs

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