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Observations of interplanetary scintillation in China

Published online by Cambridge University Press:  18 July 2013

Li-Jia Liu  and
Bo Peng
Li-Jia Liu
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences email: [email protected]
Bo Peng
Affiliation:
National Astronomical Observatories, Chinese Academy of Sciences email: [email protected]
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Abstract

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The Sun affects the Earth in multiple ways. In particular, the material in interplanetary space comes from coronal expansion in the form of solar wind, which is the primary source of the interplanetary medium. Ground-based Interplanetary Scintillation (IPS) observations are an important and effective method for measuring solar wind speed and the structures of small diameter radio sources. In this paper we will discuss the IPS observations in China.

Keywords

solar windinterplanetary scintillationobservation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S294: Solar and Astrophysical Dynamos and Magnetic Activity , August 2012 , pp. 487 - 488
Copyright
Copyright © International Astronomical Union 2013 

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