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.

Ranking academic impact of world national research institutes--by the Chinese Academy of Sciences

2013 ◽  
Vol 22 (5) ◽  
pp. 337-350 ◽  
Author(s):  
F. Xu ◽  
X. X. Li ◽  
W. Meng ◽  
W. B. Liu ◽  
J. Mingers
Keyword(s):  
Academic Impact ◽  
Research Institutes ◽  
Chinese Academy Of Sciences ◽  
Academy Of Sciences

scholarly journals Cientific Career Of The Emigratedscientists Of The Pushchinoresearch Center Ras

2019 ◽  
Vol 1 (2) ◽  
pp. 118-131 ◽  
Author(s):  
Yulia V. Mokhnacheva ◽  
Elena V. Beskaravaynaya
Keyword(s):  
Scientific Field ◽  
Research Center ◽  
Scientific Success ◽  
Russian Academy Of Sciences ◽  
Research Institutes ◽  
Academy Of Sciences ◽  
Research Institute

The article presents the results of a study of the scientific diaspora of the PushchinoResearch Center of the Russian Academy of Sciences (PRC RAS): the geography of the distribution of representatives by country and organization, as well as their scientific success and implementation. Using the example of one of the research institutes of the Research Center of the Russian Academy of Sciences, the Institute of Biochemistry and Physiology of Microorganisms of the Russian Academy of Sciences, it is shown in which directions the representatives of the scientific diaspora of this research institute are developing. As a result of the study, it was found that representatives of the foreign diaspora and their Russian colleagues work in parallel in the same scientific areas. As a result of the study, it turned out that only a little more than a quarter of all emigrating specialists achieved tangible successes in the scientific field, and more than a third altogether stopped doing science. The study is based on the integrated use of scientometric, bibliometric, bibliographic, factographic and sociological methods.

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 FON DUSHANBE CATALOGUE. RESULTS OF PROCESSING IN THE TYCHO-2 SYSTEM

2021 ◽  
Vol 34 ◽  
pp. 106-109
Author(s):  
G. Kokhirova ◽  
H. Relke ◽  
Q. Yuldoshev ◽  
Yu.I. Protsyuk ◽  
V.M. Andruk
Keyword(s):  
Northern Hemisphere ◽  
Astronomical Observatory ◽  
Astronomical Institute ◽  
National Academy Of Sciences ◽  
Main Astronomical Observatory ◽  
Digitized Images ◽  
Academy Of Sciences ◽  
M 14 ◽  
Research Institute

In the Tycho-2 catalogue system the processing of 1529 photographic plates of the FON Dushanbe project from the collection of the Institute of Astrophysics of the National Academy of Sciences of Tajikistan was completed. The photographic plates with the size of 8º×8º (30x30 cm) were exposed in the zones from -8º to + 84º in the period of 1985-1992 years. In years 2017 – 2020 the plates were digitized using a Microtek ScanMaker 1000XL Plus scanner with the resolution of 1200 dpi, so the size of the digitized images is near 13000x13000 px. Based on the results of the processing of digitized images a catalogue of equatorial coordinates α, δ and B-magnitudes of stars for the northern hemisphere of the sky was created. The catalog contains about 30 million stars and galaxies for the epoch 1988.74. The average internal accuracy of the catalogue for all objects is σαδ = ±0.32" and σB = ± 0.11 m (for stars in the range of B = 8 m -14 m the errors are σαδ = ±0.19" and σB =±0.07 m ) for equatorial coordinates and B-magnitudes respectively. The convergence between calculated and reference positions from the Tycho-2 catalogue is σαδ = ±0.07" and the convergence with photoelectric B-magnitudes is σB = ±0.16 m . Five astronomical institutions took part in the processing of the photographic plates and in the creating of the FON-Dushanbe catalogue: Institute of Astrophysics of NAS of Tajikistan; Walter Hohmann Observatory, Essen, Germany; Ulugh Beg Astronomical Institute UAS, Uzbekistan; Research Institute “Mykolaiv Astronomical Observatory”, Ukraine and Main Astronomical Observatory NASU, Ukraine.

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.

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.

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.

Sign in / Sign up

Export Citation Format

Share Document