Committee on Radio Astronomy Frequencies

The Committee on Radio Astronomy Frequencies (CRAF) is a committee of the European Science Foundation (ESF).

Frequency band allocated to the Radio Astronomy Service:

• ITU-RR allocations (+ footnotes)
• National Arrangements for Radio Astronomy different from ITU-R Radio Regulations
• Astrophysical importance of the band 182 - 185 GHz
• Threshold levels of interference detrimental to radio astronomy
• Radio Astronomy use of this band in Europe
• Threats to the Radio Astronomy Service

ITU-RR allocations (+ footnotes):

		
174.8 - 182   GHz:	EARTH EXPLORATION-SATELLITE (passive)
			INTER-SATELLITE (space-to-Earth) 5.562H
			SPACE RESEARCH (passive)


182   - 185   GHz:	EARTH EXPLORATION-SATELLITE (passive)
			RADIO ASTRONOMY
			SPACE RESEARCH (passive)
			
			5.340


185   - 190   GHz:	EARTH EXPLORATION-SATELLITE (passive)
			INTER-SATELLITE (space-to-Earth) 5.562H
			SPACE RESEARCH (passive)

National Arrangements for Radio Astronomy different from ITU-R Radio Regulations:

• Liechtenstein: no allocation but No. 5.340 applies

Astrophysical importance of the band 182 - 185 GHz

This frequency band is used for both spectral line and continuum observations.

See also: mm-Wavelength Astronomy.

Threshold levels of interference detrimental to radio astronomy spectral-line observations:

	System Sensitivity (noise fluctuations)		Threshold Interference Levels
	Temperature	Power Spectral Density	Input Power	Power Flux Density	Spectral Power Flux Density
Single Dish	2.45 mK	-255 dB(WHz-1)	-203 dBW	-137 dB(Wm-2)	-199 (Wm-2Hz-1)

Threshold levels of interference detrimental to radio astronomy continuum observations:

	System Sensitivity (noise fluctuations)		Threshold Interference Levels
	Temperature	Power Spectral Density	Input Power	Power Flux Density	Spectral Power Flux Density
Single Dish	0.048 mK	-272 dB(WHz-1)	-186 dBW	-120 dB(Wm-2)	-216 dB(Wm-2Hz-1)

NOTE:

For further details the reader is referred to ITU-R Recommendation RA769. It should, however, be noted that the observed spectral power flux densities are much lower than the harmful interference levels because they are made in the main beam of the radio astronomy antennas whereas the harmful levels correspond to reception in the sidelobes, i.e. the differences are related to the gain of the antennas. The differences can be of the order of 50 to 80 dB W m^-2 Hz^-1 (see ITU-R "Handbook on Radio Astronomy", 1995/2003, chapter 4).

In Europe, the band 182 - 185 GHz is used by the Radio Astronomy Service in:

• Spain

Threats to the Radio Astronomy Service:

Out-of-band emission from the following service:

• Inter-Satellite Service