IMPROVING THE QUASAR VLBI NETWORK FOR DATA TRANSFER WITH THE NATIONAL RESEARCH COMPUTER NETWORK OF RUSSIA
Authors:
1.
Institute of Applied Astronomy of the Russian Academy of Sciences
2.
Institute of Applied Astronomy of the Russian Academy of Sciences
3.
Institute of Applied Astronomy of the Russian Academy of Sciences
4.
National Research Centre "Kurchatov Institute"
5.
National Research Centre "Kurchatov Institute"
6.
National Research Centre "Kurchatov Institute"
Type:
Сonference article
Published:
27.12.2024
Subject area:
UDK 004.7 Связь компьютеров. Сети ЭВМ. Вычислительные сети
UDK 52 Астрономия. Геодезия
UDK 53 Физика
UDK 520 Инструменты, приборы и методы астрономических наблюдений, измерений и анализа
UDK 521 Теоретическая астрономия. Небесная механика. Фундаментальная астрономия. Теория динамической и позиционной астрономии
UDK 523 Солнечная система
UDK 524 Звезды и звездные системы. Вселенная Солнце и Солнечная система
UDK 52-1 Метод изучения
UDK 52-6 Излучение и связанные с ним процессы
GRNTI 41.00 АСТРОНОМИЯ
GRNTI 29.35 Радиофизика. Физические основы электроники
GRNTI 29.31 Оптика
GRNTI 29.33 Лазерная физика
GRNTI 29.27 Физика плазмы
GRNTI 29.05 Физика элементарных частиц. Теория полей. Физика высоких энергий
OKSO 03.06.01 Физика и астрономия
OKSO 03.05.01 Астрономия
OKSO 03.04.03 Радиофизика
BBK 2 ЕСТЕСТВЕННЫЕ НАУКИ
BBK 223 Физика
TBK 614 Астрономия
TBK 6135 Оптика
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
UDK 52 Астрономия. Геодезия
UDK 53 Физика
UDK 520 Инструменты, приборы и методы астрономических наблюдений, измерений и анализа
UDK 521 Теоретическая астрономия. Небесная механика. Фундаментальная астрономия. Теория динамической и позиционной астрономии
UDK 523 Солнечная система
UDK 524 Звезды и звездные системы. Вселенная Солнце и Солнечная система
UDK 52-1 Метод изучения
UDK 52-6 Излучение и связанные с ним процессы
GRNTI 41.00 АСТРОНОМИЯ
GRNTI 29.35 Радиофизика. Физические основы электроники
GRNTI 29.31 Оптика
GRNTI 29.33 Лазерная физика
GRNTI 29.27 Физика плазмы
GRNTI 29.05 Физика элементарных частиц. Теория полей. Физика высоких энергий
OKSO 03.06.01 Физика и астрономия
OKSO 03.05.01 Астрономия
OKSO 03.04.03 Радиофизика
BBK 2 ЕСТЕСТВЕННЫЕ НАУКИ
BBK 223 Физика
TBK 614 Астрономия
TBK 6135 Оптика
BISAC SCI004000 Astronomy
BISAC SCI005000 Physics / Astrophysics
Language:
English
Keywords:
techniques: interferometric; telescopes
Abstract (English):
This article presents the results of the phased integration of the VLBI complex ``Quasar'' into the National Research Computer Network of Russia (NIKS). The VLBI complex ``Quasar'' has implemented e-VLBI technology in Russia, enabling near real-time radio interferometric observations. This technology is critical for high-precision determination of Universal Time, which is essential for fundamental and applied space research, particularly for the GLONASS system. The complex consists of three observatories: ``Badary'' (Republic of Buryatia), ``Zelenchukskaya'' (Karachay-Cherkess Republic), and ``Svetloe'' (Leningrad Region), with a fourth under construction in Primorsky Krai. Each observatory can register data at speeds up to 16 Gbit/s, while the correlator in St. Petersburg can receive data at up to 96 Gbit/s. The current data transmission from ``Badary'' and ``Zelenchukskaya'' is limited to 2 Gbit/s, restricting the complex’s functionality. Increasing the transfer speed to 8 Gbit/s or more would significantly improve capabilities. This article details the results of the data transfer speed tests conducted during hourly sessions to the Center for Correlation Processing of RAS in the NIKS network. Additionally, the article explores options for connecting the nearby academic organizations of the IAA RAS to the NIKS network via fiber-optic cable, enhancing the overall data transmission efficiency and reliability of the VLBI complex. The integration of these observatories into NIKS is expected to enhance the ``Quasar'' VLBI complex, enabling more robust and rapid data processing for various scientific applications.
This article presents the results of the phased integration of the VLBI complex ``Quasar'' into the National Research Computer Network of Russia (NIKS). The VLBI complex ``Quasar'' has implemented e-VLBI technology in Russia, enabling near real-time radio interferometric observations. This technology is critical for high-precision determination of Universal Time, which is essential for fundamental and applied space research, particularly for the GLONASS system. The complex consists of three observatories: ``Badary'' (Republic of Buryatia), ``Zelenchukskaya'' (Karachay-Cherkess Republic), and ``Svetloe'' (Leningrad Region), with a fourth under construction in Primorsky Krai. Each observatory can register data at speeds up to 16 Gbit/s, while the correlator in St. Petersburg can receive data at up to 96 Gbit/s. The current data transmission from ``Badary'' and ``Zelenchukskaya'' is limited to 2 Gbit/s, restricting the complex’s functionality. Increasing the transfer speed to 8 Gbit/s or more would significantly improve capabilities. This article details the results of the data transfer speed tests conducted during hourly sessions to the Center for Correlation Processing of RAS in the NIKS network. Additionally, the article explores options for connecting the nearby academic organizations of the IAA RAS to the NIKS network via fiber-optic cable, enhancing the overall data transmission efficiency and reliability of the VLBI complex. The integration of these observatories into NIKS is expected to enhance the ``Quasar'' VLBI complex, enabling more robust and rapid data processing for various scientific applications.
Keywords:
techniques: interferometric; telescopes
techniques: interferometric; telescopes
1. Abramov A., Gonchar A., Evseev A., et al., 2023, Information Technologies, 12, p. 615
