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2012•International Crimean Conference Microwave and Telecommunication TechnologyRequires access

The Russian-Ukrainian VLBI Network on the basis of "Quasar-Kvo" radio telescopes and RT-22 "Simeiz"

Alexandr E Volvach, Alexander V. Ipatov, Ya. S. Yatskiv

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Abstract

In order to develop new research in radio astronomy and astrophysics, geodynamics using the method of radio interferometry with very long baselines based on RT-22 of Science Research Institute Crimean Astrophysical Observatory and radio astronomy observatories of Quasar-KVO network of Institute of Applied Astronomy, a new research tool — the Russian-Ukrainian VLBI Network, is created. With VLBI network Quasar-Simeiz the researches in cm- and mm-wavelengths are started, and the first scientific results are obtained.

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What this paper is about

In order to develop new research in radio astronomy and astrophysics, geodynamics using the method of radio interferometry with very long baselines based on RT-22 of Science Research Institute Crimean Astrophysical Observatory and radio astronomy observatories of Quasar-KVO network of Institute of Applied Astronomy, a new research tool — the Russian-Ukrainian VLBI Network, is created. With VLBI network Quasar-Simeiz the researches in cm- and mm-wavelengths are started, and the first scientific results are obtained.

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Available abstract

In order to develop new research in radio astronomy and astrophysics, geodynamics using the method of radio interferometry with very long baselines based on RT-22 of Science Research Institute Crimean Astrophysical Observatory and radio astronomy observatories of Quasar-KVO network of Institute of Applied Astronomy, a new research tool — the Russian-Ukrainian VLBI Network, is created. With VLBI network Quasar-Simeiz the researches in cm- and mm-wavelengths are started, and the first scientific results are obtained.

Key concepts: Very-long-baseline interferometry, Quasar, Astronomy, Physics, Ukrainian, Radio astronomy, Radio telescope, Interferometry

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The Russian-Ukrainian VLBI Network on the basis of "Quasar-Kvo" radio telescopes and RT-22 "Simeiz" — Research Paper | ScholarLens