The Committee on Radio Astronomy Frequencies (CRAF) is a committee of
the European Science Foundation (ESF).
79 - 81 GHz: RADIO ASTRONOMY RADIOLOCATION Amateur Amateur-satellite Space research (space-to-Earth) 5.149 81 - 84 GHz: FIXED FIXED-SATELLITE (Earth-to-space) MOBILE MOBILE-SATELLITE (Earth-to-space) RADIO ASTRONOMY Space research (space-to-Earth) 5.149 5.560A 84 - 86 GHz: FIXED FIXED-SATELLITE (Earth-to-space) 5.561A MOBILE RADIO ASTRONOMY 5.149
National Arrangements for Radio Astronomy different from ITU-R Radio Regulations
:
Astrophysical importance of the band 81 - 84 GHz
See also: mm-Wavelength Astronomy.
| System Sensitivity (noise fluctuations) | Threshold Interference Levels | ||||
| Temperature | Power Spectral Density | Input Power | Power Flux Density | Spectral Power Flux Density | |
| Single Dish | 2.87 mK | -254 dB(WHz-1) | -204 dBW | -144 dB(Wm-2) | -204 dB(Wm-2Hz-1) |
| System Sensitivity (noise fluctuations) | Threshold Interference Levels | ||||
| Temperature | Power Spectral Density | Input Power | Power Flux Density | Spectral Power Flux Density | |
| Single Dish | 0.043 mK | -273 dB(WHz-1) | -186 dBW | -127 dB(Wm-2) | -225 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 81 - 84 GHz is used by the Radio Astronomy Service in:
Sharing problems with the following services:
Out-of-band emission from the following services: