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The IPS work in Beijing astronomical observatory

  • IPS and Other Remote Sensing Measurements
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Abstract

This article describes the IPS work in the Beijing astronomical observatory including the hardware and software of the instrument and some theoretical research.

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References

  • Ma G.Y. 1993a A Preliminary Computation Result of Plasma Irregularities in Solar WindC.Y.Jiang et. al., ISPR' 93 Beijing, CHINA 259.

  • 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 Astrophycis

  • Purvis, A. et al.: 1987, ‘The Cambridge IPS survey at 81.5 MHz’,Mon. Not. R. Astr. Soc. 229, 589.

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  • Qiu Yuhai: 1993, ‘Software for IPS Work and IPS data Hadling 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 

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The project is supported by the China National Nature Science Fundation under the program 49391400

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Yuhai, Q. The IPS work in Beijing astronomical observatory. Astrophys Space Sci 243, 255–258 (1996). https://doi.org/10.1007/BF00644065

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  • DOI: https://doi.org/10.1007/BF00644065

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