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PUL VLBI Analysis Center
at Pulkovo Observatory |
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PUL VLBI Analysis Center
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VLBI World
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An IVS VLBI Analysis Center at the Central Astronomical Observatory at Pulkovo
of the Russian Academy of Sciences, also widely known as Pulkovo Observatory,
has been organized in September 2006. It's IVS acronym is PUL.
The center is a part of the
Pulkovo EOP and Reference Systems Analysis Center (PERSAC).
The main topics of our activity are:
- Improvement of the International Celestial Reference Frame (ICRF),
including investigations of radio source catalogues, constructing combined
catalogues, investigation of the ICRF stability, investigation of radio source
structure and its variability.
- Investigation of EOP, station position and baseline length time series.
- Comparison of VLBI products with other space geodesy techniques.
Staff of the PUL VLBI Analysis Center:
- Dr.Sci. Zinovy Malkin, malkin@gao.spb.ru
- Ms. Natalia Miller, natm@gao.spb.ru
- Ms. Elena Popova, m02pea@hotmail.com
This statistics is based on the PUL data base of NGS cards mainly obtained
from the CDDIS IVS Data Center.
The statistics is related to X-band cards only.
Results of our VLBI data analysis can be found at the
Pulkovo EOP and Reference Systems
Analysis Center (PERSAC) page.
Forthcoming mutual events of planets and astrometric radio sources are
listed here.
Publications and presentations of the PUL VLBI Analysis Center
can be found at the personal web pages of VLBI AC staff members.
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Contact:
Zinovy Malkin, malkin@gao.spb.ru
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Pulkovo EOP and Reference Systems Analysis Center (PERSAC)
Pulkovo Observatory homepage
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Originated on 30 Sep 2006
Last updated on 22 Apr 2010
Feedback is welcome!