The Committee on Radio Astronomy Frequencies (CRAF) is a committee of
the European Science Foundation (ESF).
Radio observatories operating in Russia:
In Russia all frequency bands below 150 GHz allocated to the Radio Astronomy Service are used by radio astronomy observatories in Russia. In addition some frequency bands are used for a long time according to local notifications. Several bands used for Very Long Baseline Interferometry, VLBI, have national notifications.
This band is used by the Pushchino Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the Pushchino Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Pushchino and Zimenki :
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This band is used by the radio observatories at Pushchino and Zimenki:
Radio astronomical quality of the band:
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This band is used by the Zimenki Radio Observatory:
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This band is used by the radio observatories at Kalyazin and Zimenki:
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This band is used by the radio observatories at Zelenchukskaya and Zimenki:
Radio astronomical quality of the band:
Reason:
This band is used by the radio observatories at Kalyazin, Pushchino, Zelenchukskaya and Zimenki:
Radio astronomical quality of the band:
Reason: unwanted emission from satellite communications.
This band is used by the radio observatories at Kalyazin, Pushchino, Zelenchukskaya and Zimenki:
Radio astronomical quality of the band:
Reason:
This band is used by the radio observatories at Kalyazin, Pushchino, Zelenchukskaya and Zimenki:
Radio astronomical quality of the band:
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This band is used by the Zimenki Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Kalyazin, Pushchino, Zelenchukskaya and Zimenki:
Radio astronomical quality of the band:
Reason:
This band is used by the radio observatories at Kalyazin, Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
Reason:
This band is used by the radio observatories at Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
Reason:
This band is used by the Zelenchukskaya Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Kalyazin, Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
This band is used by the radio observatories at Kalyazin, Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
This band is used by the radio observatories at Badari, Kalyazin, Pushchino, Svetloe and Zelenchukskaya:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Badari, Kalyazin, Pushchino, Svetloe and Zelenchukskaya:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Badari, Kalyazin, Pushchino, Svetloe and Zelenchukskaya:
Radio astronomical quality of the band:
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This band is used by the radio observatories at Dmitrov, Kalyazin, Pushchino and Zelenchukskaya:
Radio astronomical quality of the band:
This band is used by the Dmitrov Radio Observatory:
This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the Pushchino Radio Observatory:
Radio astronomical quality of the band:
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This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
Reason:
This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
This band is used by the Dmitrov Radio Observatory:
Radio astronomical quality of the band:
Radio astronomical quality of the other bands used:
Other bands used by the Radio Astronomy Service in Russia:
by the Badary Radio Observatory:
by the Pushchino Radio Observatory:
by the Zelenchukskaya Radio Observatory:
By the radio observatories at Badari, Zelenchukskaya and Svetloe:
The following radio astronomy stations take part in Very Long Baseline Interferometry: