An analysis of fine structures in a solar radio burst at 10 cm and a coexisting hard X-ray flare

1999 ◽  
Vol 23 (2) ◽  
pp. 208-220 ◽  
Author(s):  
Da-Wei Tian ◽  
Zheng-min Gao ◽  
Qi-jun Fu
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Solar Radio Burst ◽  
X Ray ◽  
Fine Structures

scholarly journals Occurrence of Solar Radio Burst Fine Structures in 1–7.6 GHz Range Associated with CME Events

2004 ◽  
Vol 2004 (IAUS226) ◽  
pp. 101-107
Author(s):  
Yihua Yan ◽  
Yuying Liu ◽  
Zhijun Chen ◽  
Qijun Fu ◽  
Chengming Tan ◽  
...  
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Solar Radio Burst ◽  
Fine Structures

The fine structures in the solar radio burst at 2 cm waveband

1992 ◽  
Vol 16 (3) ◽  
pp. 359
Author(s):  
Gao Zheng-min ◽  
Li Zi-ying ◽  
Huo Cai-ping ◽  
Fan Ying
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Solar Radio Burst ◽  
Fine Structures

The quasi-periodic fine structures in a solar radio burst at 3.2 cm wavelength on 23 May 1990

1992 ◽  
Vol 16 (1) ◽  
pp. 78-83
Author(s):  
Qin Zhi-hai ◽  
Li Chun-sheng ◽  
Wei Shuang-ling ◽  
Chen Yun-xia
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Solar Radio Burst ◽  
Fine Structures

scholarly journals Imaging spectroscopy of solar radio burst fine structures

2017 ◽  
Vol 8 (1) ◽  
Author(s):  
E. P. Kontar ◽  
S. Yu ◽  
A. A. Kuznetsov ◽  
A. G. Emslie ◽  
B. Alcock ◽  
...  
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Imaging Spectroscopy ◽  
Solar Radio Burst ◽  
Fine Structures

scholarly journals Publisher Correction: Imaging spectroscopy of solar radio burst fine structures

2018 ◽  
Vol 9 (1) ◽  
Author(s):  
E. P. Kontar ◽  
S. Yu ◽  
A. A. Kuznetsov ◽  
A. G. Emslie ◽  
B. Alcock ◽  
...  
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Imaging Spectroscopy ◽  
Solar Radio Burst ◽  
Fine Structures

scholarly journals Evidence for the Transfer of Corpuscles to Distant Parts of the Sun Following a Solar Radio Burst

1961 ◽  
Vol 14 (4) ◽  
pp. 540 ◽  
Author(s):  
RF Mullaly
Keyword(s):  
Radio Burst ◽  
Solar Radio ◽  
Brightness Distribution ◽  
Solar Radio Burst ◽  
The Sun ◽  
Time Intervals ◽  
The Past ◽  
Grating Interferometer ◽  
Half Power ◽  
East West

The brightness distribution of 21-cm radiation over the Sun's surface has been studied for the past four years with the Christiansen crossed-grating interferometer (Christiansen et al. 1961) at Fleurs near Sydney. The observations described here were made using one arm of this cross as a simple grating interferometer, providing a transit instrument with a fan beam of about 2' of arc resolution to half-power points in the east-west direction and very low resolution north-south. The Sun was scanned repeatedly from east to west at time intervals of approximately 4 min.

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