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Helio-Geodynamic Polygon “Simeiz–Katsiveli” for Positioning, Navigation, and Timing Support

A. E. Volvach, A. I. Dmitrotsa, D. I. Neyachenko

Transactions of IAA RAS, issue 37, 55–58 (2016)

Keywords: Earth Orientation Parameters, satellite laser ranging, very long baseline interferometry, co-location.

Abstract

The “Simeiz–Katsiveli” helio-geodynamic polygon is created to study geodynamic phenomena and the impact of the Sun’s parameters on the state of the Earth's ecosystem. There are the following observational tools at its disposal: the “Simeiz” VLBI station based on the RT-22 radio telescope, two satellite laser ranging stations (“Simeiz-1873” and “Katsively-1893”), two GPS/GLONASS stations (“GPS-CrAO” and “Katsively”) and a Solar activity monitoring station with its radio telescopes RT-2, RT-3 and RT-M, a part of the Sun Service international network. Adjoining the fourth RT-22 Observatory “Simeiz” to the observations of the VLBI network “Quasar-KVO” gives the opportunity to obtain more accurate and reliable data in order to create the terrestrial reference systems and for the fundamental scientific research.

Citation

Text

BibTeX

RIS

A. E. Volvach, A. I. Dmitrotsa, D. I. Neyachenko. Helio-Geodynamic Polygon “Simeiz–Katsiveli”  for Positioning, Navigation, and Timing Support // Transactions of IAA RAS. — 2016. — Issue 37. — P. 55–58.

@article{volvach2016,
  abstract = {The “Simeiz–Katsiveli” helio-geodynamic polygon is created to study geodynamic phenomena and the impact of the Sun’s parameters on the state of the Earth's ecosystem. There are the following  observational tools at its disposal: the “Simeiz” VLBI station based on the RT-22 radio telescope, two satellite laser ranging stations (“Simeiz-1873” and “Katsively-1893”), two GPS/GLONASS stations (“GPS-CrAO” and “Katsively”) and a Solar activity monitoring station with its radio telescopes RT-2, RT-3 and RT-M, a part of the Sun Service international network. Adjoining the fourth RT-22 Observatory “Simeiz” to the observations of the VLBI network “Quasar-KVO” gives the opportunity to obtain more accurate and reliable data in order to create the terrestrial reference systems and for the fundamental scientific research.},
  author = {A.~E. Volvach and A.~I. Dmitrotsa and D.~I. Neyachenko},
  issue = {37},
  journal = {Transactions of IAA RAS},
  keyword = {Earth Orientation Parameters, satellite laser ranging, very long baseline interferometry, co-location},
  pages = {55--58},
  title = {Helio-Geodynamic Polygon “Simeiz–Katsiveli”  for Positioning, Navigation, and Timing Support},
  url = {http://iaaras.ru/en/library/paper/1558/},
  year = {2016}
}

TY  - JOUR
TI  - Helio-Geodynamic Polygon “Simeiz–Katsiveli”  for Positioning, Navigation, and Timing Support
AU  - Volvach, A. E.
AU  - Dmitrotsa, A. I.
AU  - Neyachenko, D. I.
PY  - 2016
T2  - Transactions of IAA RAS
IS  - 37
SP  - 55
AB  -  The “Simeiz–Katsiveli” helio-geodynamic polygon is created to study
geodynamic phenomena and the impact of the Sun’s parameters on the
state of the Earth's ecosystem. There are the following
observational tools at its disposal: the “Simeiz” VLBI station based
on the RT-22 radio telescope, two satellite laser ranging stations
(“Simeiz-1873” and “Katsively-1893”), two GPS/GLONASS stations (“GPS-
CrAO” and “Katsively”) and a Solar activity monitoring station with
its radio telescopes RT-2, RT-3 and RT-M, a part of the Sun Service
international network. Adjoining the fourth RT-22 Observatory
“Simeiz” to the observations of the VLBI network “Quasar-KVO” gives
the opportunity to obtain more accurate and reliable data in order to
create the terrestrial reference systems and for the fundamental
scientific research.
UR  - http://iaaras.ru/en/library/paper/1558/
ER  -