Hostname: page-component-586b7cd67f-2plfb Total loading time: 0 Render date: 2024-11-25T20:39:22.795Z Has data issue: false hasContentIssue false

A CME and Related Phenomena on 2003 October 26

Published online by Cambridge University Press:  03 June 2005

Zongjun Ning
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: [email protected]
C. Fang
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: [email protected]
M. D. Ding
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: [email protected]
C.-T. Yeh
Affiliation:
Department of Astronomy, Nanjing University, Nanjing 210093, China email: [email protected]
H. Li
Affiliation:
Purple Mountain Observatory, Nanjing 210008, China
Y. N Xu
Affiliation:
Purple Mountain Observatory, Nanjing 210008, China
Y. Zhang
Affiliation:
Chinese National Observatory, Beijing 100021, China
C. M. Tan
Affiliation:
Chinese National Observatory, Beijing 100021, China
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

We present the observational results of the solar bursts on the band of 1-80 GHz (NORH) associated with both a CME and a flare on Oct. 26 2003. This event shows two parts of radio bursts in the time profile. The first part is associated with an X1.2 flare. However, the following part seams related to both the flare and the CME, as the radio emission is enhanced while the ${\rm H}\alpha$ is decreasing. Thus, these two parts of radio bursts may originate from different physical processes, i.e., flare and CME shock. A primary study is performed on the difference between this two parts.To search for other articles by the author(s) go to: http://adsabs.harvard.edu/abstract_service.html

Type
Contributed Papers
Copyright
© 2005 International Astronomical Union