No CrossRef data available.
Article contents
The IPS Work in Beijing Astronomical Observatory
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.
This article describes the IPS work in the Beijing astronomical observatory including the hardware and software of the instrument and some theoretical research.
Information
- Type
- IPS and Other Remote Sensing Measurements
- Information
- International Astronomical Union Colloquium , Volume 154: Solar and Interplanetary Transients , 1996, pp. 255 - 258
- Copyright
- Copyright © Kluwer 1997
References
Ma, G.Y.
1993a A Preliminary Computation Result of Plasma Irregularities in Solar Wind
Jiang, C.Y.
et. al., ISPR’ 93
Beijing, China
259.Google Scholar
Ma, G.Y., Wang, J.L.:1994, ‘Research of solar Wind by Observations of Radio Wave Propagation’, Progress in Astronomy (China)
1.12., 30.Google Scholar
Ma, G.Y. .:1993b, ‘A Study of Interplanetary Scintillation and Its Application’, Thesis for PH.D. Degree, in AstrophysicsGoogle Scholar
Purvis, A.
et al.:1987, ‘The Cambridge IPS survey at 81.5 MHz’,Mon. Not. R .Astr. Soc.
229, 589.CrossRefGoogle Scholar
Qiu Yuhai, ,: 1993, ‘Software for IPS Work and IPS data Handling Sub-Package under IRAF’The publication of Beijing astronomical observatory .20, 82.Google Scholar
Wang, S.G.
et al.:1985, ‘The Miyun Metre-wave Aperture Synthesis Radio Telescope’,Acta Astrophysics. Sin.
10.5., 245.Google Scholar
You have Access