Hostname: page-component-848d4c4894-cjp7w Total loading time: 0 Render date: 2024-07-08T01:37:25.396Z Has data issue: false hasContentIssue false
  • English
  • Français

IPS Observations at Miyun Station, BAO

Published online by Cambridge University Press:  13 May 2016

X.Z. Zhang  and
J.H. Wu
X.Z. Zhang
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China & National Astronomical Observatories, CAS, Beijing 100012, China
J.H. Wu
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100012, China & National Astronomical Observatories, CAS, Beijing 100012, China

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.

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.

Type
Session VI: The Solar Wind and Heliosphere
Information
Symposium - International Astronomical Union , Volume 203: Recent Insights into the Physics of the Sun and Heliosphere: Highlights from Soho and Other Space Missions , 2001 , pp. 580 - 582
Copyright
Copyright © Astronomical Society of the Pacific 2001 

References

Manoharan, P. K. and Ananthakrishnan, S.: 1990, ‘Determination of solar-wind velocities using single-station measurements of interplanetary scintillation’, MNRAS, 244, 691.Google Scholar
Pramesh Rao, A., Bhandari, S. M. and Ananthakrishnan, S.: 1974, ‘Observations of Interplanetary Scintillations at 327 MHz’, Aust. J. Phys., 27, 105.CrossRefGoogle Scholar
Oberio, D.: 2000, , p95.Google Scholar
Wu, J.H., Zhang, X.Z. & Zheng, Y.J., 2000, Ap&SS, in press.Google Scholar
Wang, S.G. 1987, Publications of BAO, p1.Google Scholar