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Observations of microwave type-U bursts
Wang, M ; Fu, QJ ; Xie, RX ; Huang, GL ; Duan, CC
Source PublicationSOLAR PHYSICS
AbstractTwo microwave type-U bursts observed with the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) are described and analysed in this paper. The microwave type-U bursts have very short durations (about 200 ms), narrow bandwidth. high-frequency drift rates of the ascending and descending branches, and a high degree of circular polarization (80%). The sense of polarization remains the same from the ascending to the descending branch.
KeywordRadio-bursts Solar
Subject AreaAstronomy & Astrophysics
Document Type期刊论文
Recommended Citation
GB/T 7714
Wang, M,Fu, QJ,Xie, RX,et al. Observations of microwave type-U bursts[J]. SOLAR PHYSICS,2001,199(1):157—164.
APA Wang, M,Fu, QJ,Xie, RX,Huang, GL,&Duan, CC.(2001).Observations of microwave type-U bursts.SOLAR PHYSICS,199(1),157—164.
MLA Wang, M,et al."Observations of microwave type-U bursts".SOLAR PHYSICS 199.1(2001):157—164.
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