Abstract
IPS observations have recently begun at Miyun Station, Beijing Astronomical Observatory. This paper briefly describes the radio telescope at Miyun Station, discusses the observation and the data reduction procedures, and presents the preliminary results of observations on IPS source 3C48.
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References
Manoharan, P.K. and Ananthakrishnan, S.: 1990, Determination of solar-wind velocities using single-station measurements of interplanetary scintillation, Mon. Not. R. Astron. Soc. 244, 691–695.
Ma, G.: 1993, PhD Thesis, Beijing Astronomical Observatory, Chinese Academy of Sciences, p. 45.
Pramesh Rao, A., Bhandari, S.M. and Ananthakrishnan, S.: 1974, Observations of Interplanetary Scintillations at 327 MHz, Aust. J. Phys. 27, 105–120.
Oberio, D.: 2000, PhD Thesis, NCRA, Tata Institute of Fundamental Research, India, p. 95.
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Wu, J., Zhang, X. & Zheng, Y. IPS Observations at Miyun Station, BAO. Astrophysics and Space Science 278, 189–192 (2001). https://doi.org/10.1023/A:1013106829146
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DOI: https://doi.org/10.1023/A:1013106829146