Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-23T02:01:26.393Z Has data issue: false hasContentIssue false

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
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.

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