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Radio Behavior of Solar Post-Flare Loops

Published online by Cambridge University Press:  01 November 2006

M. Wang
Affiliation:
Yunnan Observatory, National Astronomical Observatories, CAS, Kunming 650011, China
R. X. Xie
Affiliation:
Yunnan Observatory, National Astronomical Observatories, CAS, Kunming 650011, China
H. D. Chen
Affiliation:
Yunnan Observatory, National Astronomical Observatories, CAS, Kunming 650011, China
Y. H. Yan
Affiliation:
National Astronomical Observatories, CAS, Beijing 100012, China
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Abstract

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The spectral and source characteristics of a complex radio burst observed with the spectrometers of China and the Nobeyama Radio Heliograph are analyzed. This burst presents two separate burst peaks occurred in different frequency range (broad-band microwave and narrow-band decimeter wavelengths). We stress that the late phase radio bursts in decimeter wavelength corresponding to the post-flare loops may be the radio homologous flare.

Type
Contributed Papers
Copyright
© 2006 International Astronomical Union