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Observations of interplanetary scintillation with a single-station mode at Urumqi
Liu, Li-Jia1; Zhang, Xi-Zhen1; Li, Jian-Bin1; Manoharan, P. K.2; Liu, Zhi-Yong3; Peng, Bo1
2010-06-01
Source PublicationRESEARCH IN ASTRONOMY AND ASTROPHYSICS
Volume10Issue:6Pages:577-586
AbstractThe Sun affects physical phenomena on Earth in multiple ways. In particular, the material in interplanetary space comes from coronal expansion in the form of inhomogeneous plasma flow (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. We discuss one mode of ground-based single-station observations: Single-Station Single-Frequency (SSSF) mode. To study the SSSF mode, a new system has been established at Urumqi Astronomical Observatory (UAO), China, and a series of experimental observations were successfully carried out from May to December, 2008.
KeywordMethods: Data Analysis Solar Wind Methods: Numerical
Indexed BySCI
Language英语
WOS IDWOS:000279087400007
Citation statistics
Cited Times:4[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/7756
Collection射电天文研究部
Affiliation1.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
2.TIFR NCRA, Radio Astron Ctr, Ooty 643001, India
3.Chinese Acad Sci, Natl Astron Observ, Urumqi Observ, Urumqi 830011, Peoples R China
Recommended Citation
GB/T 7714
Liu, Li-Jia,Zhang, Xi-Zhen,Li, Jian-Bin,et al. Observations of interplanetary scintillation with a single-station mode at Urumqi[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2010,10(6):577-586.
APA Liu, Li-Jia,Zhang, Xi-Zhen,Li, Jian-Bin,Manoharan, P. K.,Liu, Zhi-Yong,&Peng, Bo.(2010).Observations of interplanetary scintillation with a single-station mode at Urumqi.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,10(6),577-586.
MLA Liu, Li-Jia,et al."Observations of interplanetary scintillation with a single-station mode at Urumqi".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 10.6(2010):577-586.
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