No CrossRef data available.
Article contents
Effects of RFI on Solar Microwave Bursts Observed with Hightime Resolution
Published online by Cambridge University Press: 12 April 2016
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.
Solar microwave burst observations with high time resolution (~ 1 ms) are important but difficult to make. It is shown by the experiments of radiometer at wavelength 21 cm on 1 ms time scale that some ultrafast time structures in microwaves, which includes spike impulses, switch-on and switch-off structures, etc., may not be from solar emission but from RFI (radio-frequency interference) or from radiometer itself. Because of the uncertainty at 21 cm and other several wavelengths, we suggest that joint observations of the solar microwave bursts on 1 ms time scale should be carried out on the peak years of the 22nd solar activity cycle.
- Type
- Radio Frequency Interference
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 1991
References
(3)
Kaufmann, P., Strauss, F. M.
Opher, R. and LaPorte, C., 1980, Astron. Astrophvs., 87. 58–62.Google Scholar
(5)
Xianhan, Luo, Yuanyi, Yan, Deyi, Yao, Li, Zhou, Weixue, Zhang and Xi, Lu, 1984. Publications of the Beijing Astronomical Observatory. 7.101–105.Google Scholar
(6)
Hanming, Hu, Songquan, Lu, Yuanfang, Gong, Shuobiao, Shi and Qiongzhen, Shang, 1988, Publications of Yunnan Observatory. No. 1, pp.39–44.Google Scholar
(7)
Shuchen, Ji, Ruixiang, Xie and Fan, Zhang, 1988, Publications of Yunnan Observatory. No. 1, p.92.Google Scholar
You have
Access