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On the Initial Phase of Solar Radio Burst Event on 23 September 1998

Published online by Cambridge University Press:  13 May 2016

Y. Yan ,
Q. Fu ,
H. Aurass ,
S. Lesovoi ,
A. Altyntsev ,
Y. Liu ,
Z. Chen  and
H. Ji
Y. Yan
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Q. Fu
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
H. Aurass
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, D-14482 Potsdam, Germany
S. Lesovoi
Affiliation:
Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Sciences, 664033, Irkutsk, P.O. Box 4026, Russia
A. Altyntsev
Affiliation:
Institute of Solar-Terrestrial Physics, Siberian Division, Russian Academy of Sciences, 664033, Irkutsk, P.O. Box 4026, Russia
Y. Liu
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
Z. Chen
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
H. Ji
Affiliation:
Beijing Astronomical Observatory, Chinese Academy of Sciences, Beijing 100012, China National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

Abstract

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On 23 September 1998 there was a 3B/M7.1 flare event starting at 06:40 UT with more than 100 minute duration radio bursts of 1134 sfu peak flux at 2840 MHz and accompanying a CME. In this paper, the event is analyzed with the data observed by Beijing Astronomical Observatory (BAO), OSRA-Tremsdorf (AIP) and SSRT-ISTP. In particular, we compare the fine structures (FS) during the triggering phase revealed in different regimes and discuss their implications.

Type
Session III: Active Region Structure and Dynamics
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 338 - 340
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

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