NAOC Open IR  > 射电天文研究部
Simulation of interplanetary scintillation with SSSF and SSDF mode
Liu LiJia; Peng Bo
2010
Source PublicationSCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
Volume53Issue:1Pages:187-192
AbstractThe sun has the biggest effect on the Earth in many ways. Observing the solar wind is an important method to study the solar-earth environment. Ground-based interplanetary scintillation observations are an effective method of monitoring solar wind speed, studying the random fluctuations of the interplanetary plasma and the structures of radio sources. Two modes of single-station observations, namely, single station-single frequency (SSSF) and single station dual-frequency (SSDF), are briefly introduced and numerically simulated in this paper. The SSSF mode are easier to carry out and has been widely used. Although the observing system and data processing system of the SSDF mode are more complicated, it can measure the solar wind speed more accurately. A new SSDF system is under construction in Miyun, NAOC ( the National Astronomical Observatories, Chinese Academy of Sciences), with a 50 m telescope, which will serve the Meridian Project, and this paper is devoted to preparing for this new system.
KeywordInterplanetary Scintillation Single station-Single Frequency Single Station Dual-frequency Simulation
DOI10.1007/s11433-010-0076-3
Indexed BySCI
Language英语
WOS IDWOS:000276490300028
Citation statistics
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/7795
Collection射电天文研究部
AffiliationChinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
Recommended Citation
GB/T 7714
Liu LiJia,Peng Bo. Simulation of interplanetary scintillation with SSSF and SSDF mode[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2010,53(1):187-192.
APA Liu LiJia,&Peng Bo.(2010).Simulation of interplanetary scintillation with SSSF and SSDF mode.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,53(1),187-192.
MLA Liu LiJia,et al."Simulation of interplanetary scintillation with SSSF and SSDF mode".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 53.1(2010):187-192.
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