scholarly journals The Sino-German λ6cm polarization survey of the Galactic plane

2012 ◽  
Vol 10 (H16) ◽  
pp. 394-394
Author(s):  
J. L. Han ◽  
W. Reich ◽  
X. H. Sun ◽  
X. Y. Gao ◽  
L. Xiao ◽  
...  
Keyword(s):  
Sea Level ◽  
Radio Telescope ◽  
High Frequency ◽  
Galactic Plane ◽  
Astronomical Observatory ◽  
Processing Methods ◽  
Dual Channel ◽  
Chinese Academy Of Sciences ◽  
Academy Of Sciences

After Prof. R. Wielebinski visited China in 1999, we started to plan the Sino-German λ6 cm polarization survey of the Galactic plane, using the Urumqi 25-m radio telescope of Xinjiang (formerly Urumqi) Astronomical Observatory, Chinese Academy of Sciences. It is a high-frequency complement of previous Effelsberg 21-cm and 11-cm surveys, using the same observing and processing methods. The telescope is located at an altitude of 2029 m above sea level at geographic longitude of 87°E and latitude 43°N. The dual-channel λ6 cm receiver with a polarimeter and a bandwidth of 600 MHz was designed by O. Lochner and constructed at the MPIfR in Germany with involvements by the Urumqi engineers M.Z. Chen and J. Ma. In August 2004, the receiver was installed at the secondary focus of the Urumqi 25-m telescope.

Decades of Chinese Solar and Geophysical Data

2018 ◽  
Vol 13 (S340) ◽  
pp. 71-72 ◽  
Author(s):  
Yan Yan ◽  
Zhan-Le Du ◽  
Hua-Ning Wang ◽  
Han He ◽  
Juan Guo ◽  
...  
Keyword(s):  
Solar Flares ◽  
Data Exchange ◽  
Astronomical Observatory ◽  
Geophysical Data ◽  
Radio Bursts ◽  
Ionospheric Storm ◽  
Solar Radio Bursts ◽  
Chinese Academy Of Sciences ◽  
Forecast Data ◽  
Academy Of Sciences

AbstractThe Chinese Solar and Geophysical Data (CSGD) was first issued at the Beijing Astronomical Observatory, Chinese Academy of Sciences (now the headquarter of the National Astronomical Observatories, Chinese Academy of Sciences) in 1971, when China’s satellite-industry was booming. CSGD covers the observational data (observations of the sunspots, solar flares, solar radio bursts, ionospheric storm and geomagnetic storm) from a couple of domestic observatories and the forecast data. The compiler of CSGD still keeps the data exchange with other institutes worldwide. The type of the dataset includes texts, tables, figures and so on. Up to now, we have electronized all the historic archives, making them easily accessible to people who are interested in them.

scholarly journals A brief history of Regional Warning Center China (RWC-China)

2018 ◽  
Vol 9 (1) ◽  
pp. 41-47 ◽  
Author(s):  
Han He ◽  
Huaning Wang ◽  
Zhanle Du ◽  
Xin Huang ◽  
Yan Yan ◽  
...  
Keyword(s):  
Astronomical Observatory ◽  
Space Environment ◽  
Short Term ◽  
Activity Prediction ◽  
International Space ◽  
Chinese Academy Of Sciences ◽  
History Of ◽  
Academy Of Sciences ◽  
Environment Service ◽  
Terrestrial Data

Abstract. Solar-terrestrial prediction services in China began in 1969 at the Beijing Astronomical Observatory (BAO), Chinese Academy of Sciences (CAS). In 1990, BAO joined the International URSIgram and World Days Service (IUWDS) and started solar-terrestrial data and prediction interchanges with other members of IUWDS. The short-term solar activity prediction service with standard URSIgram codes began in January 1991 at BAO, and forecasts have been issued routinely every weekday from then on. The Regional Warning Center Beijing (RWC-Beijing) of IUWDS was officially approved in China in 1991 and was formally established in February 1992. In 1996, the IUWDS was changed to the current name, the International Space Environment Service (ISES). In 2000, the RWC-Beijing was renamed RWC-China according to ISES requirements. In 2001, the National Astronomical Observatories, CAS (NAOC) was established. All the solar-terrestrial data and prediction services of BAO were taken up by NAOC. The headquarters of RWC-China is located on the campus of NAOC.

EDITORIAL

2013 ◽  
Vol 02 (02) ◽  
pp. 3-3
Author(s):  
Kok Khoo Phua
Keyword(s):  
Astronomical Observatory ◽  
Asia Pacific ◽  
Research Institutes ◽  
Chinese Academy Of Sciences ◽  
Astronomical Research ◽  
Academy Of Sciences ◽  
Astronomy And Astrophysics ◽  
Research Institute

In this issue of the Asia Pacific Physics Newsletter (APPN), we introduce four Astronomical Research Institutes in Asia Pacific: the Australian Astronomical Observatory, National Astronomical Research Institute of Thailand, Shanghai Astronomical Observatory, Chinese Academy of Sciences and Institute of Astronomy and Astrophysics, Academia Sinica, Taiwan.

scholarly journals Shanghai Astronomical Observatory, Chinese Academy of Sciences

2013 ◽  
Vol 02 (02) ◽  
pp. 74-75
Keyword(s):  
Astronomical Observatory ◽  
Chinese Government ◽  
Chinese Academy Of Sciences ◽  
Academy Of Sciences

Shanghai Astronomical Observatory (SHAO) of the Chinese Academy of Sciences (CAS), was established in 1962 following the amalgamation of the former Xu Jiahui and Sheshan observatories, which were founded by the French Mission Catholique in 1872 and 1900, respectively. Both came under the Chinese government jurisdiction in 1950.

scholarly journals Correction: Fu, N.; et al. The Two-Parts Step-by-Step Ionospheric Assimilation Based on Ground-Based/Spaceborne Observations and Its Verification. Remote Sens. 2019, 11, 1172

2019 ◽  
Vol 11 (17) ◽  
pp. 2006
Author(s):  
Naifeng Fu ◽  
Peng Guo ◽  
Mengjie Wu ◽  
Yong Huang ◽  
Xiaogong Hu ◽  
...  
Keyword(s):  
Astronomical Observatory ◽  
Oral Examination ◽  
Chinese Academy Of Sciences ◽  
Academy Of Sciences

Because our organization pays great attention to the order of the unit names in the signature of the paper, the papers in which the first affiliation of the article is “Shanghai Astronomical Observatory of Chinese Academy of Sciences, Shanghai, 200030, China” are counted as the first condition for the doctoral graduation oral examination [...]

scholarly journals Study Of Atmospheric Absorption And PWV In The Suffa Plateau (Uzbekistan)

2021 ◽  
Vol 03 (03) ◽  
pp. 28-33
Author(s):  
D.A. Raupov ◽  
Keyword(s):  
Sea Level ◽  
Radio Telescope ◽  
Astronomical Observatory ◽  
Construction Site ◽  
Atmospheric Absorption ◽  
Atmospheric Radio

Radio Astronomical Observatory of Suffa, and new proposals for radioastroclimatic (seeing) studies for atmospheric radio prediction are described. The paper presents the results of many-year (2015-2020) and seasonal observations of the astroclimate at the construction site of the RT-70 radio telescope on the Suffa plateau (an altitude of 2400 m above sea level). Observations were carried out automatically every 10 minutes throughout the year, starting from November 2014.

scholarly journals Preface to the Interfacial Science Developments at the Chinese Academy of Sciences Virtual Special Issue

Langmuir ◽  
2020 ◽  
Vol 36 (41) ◽  
pp. 12087-12087 ◽  
Author(s):  
Yilin Wang ◽  
Shaoyi Jiang ◽  
Zhan Chen ◽  
Shu-Hong Yu ◽  
Gilbert Walker
Keyword(s):  
Special Issue ◽  
Interfacial Science ◽  
Chinese Academy Of Sciences ◽  
Academy Of Sciences

Two new species of the spider genus Pholcus Walckenaer, 1805 (Araneae: Pholcidae) from Pakistan

Zootaxa ◽  
2020 ◽  
Vol 4820 (1) ◽  
pp. 177-185
Author(s):  
TIANQI LAN ◽  
ZHIYUAN YAO ◽  
ABID ALI ◽  
GUO ZHENG ◽  
SHUQIANG LI
Keyword(s):  
New Species ◽  
Species Group ◽  
Male And Female ◽  
Female Type ◽  
Chinese Academy Of Sciences ◽  
Two New Species ◽  
Academy Of Sciences ◽  
Gilgit Baltistan ◽  
First Time ◽  
Beijing China

The genus Pholcus Walckenaer, 1805 is reported from Pakistan for the first time. Two new species of the Pholcus nenjukovi species-group are described: Pholcus hamuchal Yao & Li sp. nov. (Gilgit Baltistan, male and female) and Pholcus kalam Yao & Li sp. nov. (Khyber Pakhtunkhwa, male and female). Type material is deposited in the Institute of Zoology, Chinese Academy of Sciences (IZCAS) in Beijing, China.

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