The Committee on Radio Astronomy Frequencies (CRAF) is a committee of
the European Science Foundation (ESF).
122.25 - 123 GHz: FIXED INTER-SATELLITE MOBILE 5.558 Amateur 5.138 123 - 126 GHz: FIXED-SATELLITE (space-to-Earth) MOBILE-SATELLITE (space-to-Earth) RADIONAVIGATION RADIONAVIGATION-SATELLITE Radio astronomy 5.554 126 - 130 GHz: FIXED-SATELLITE (space-to-Earth) MOBILE-SATELLITE (space-to-Earth) RADIONAVIGATION RADIONAVIGATION-SATELLITE Radio astronomy 5.562D 5.149 5.554
Astrophysical importance of the band 123 - 126 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 | 2.88 mK | -254 dB(WHz-1) | -204 dBW | -140 dB(Wm-2) | -201 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 | 0.034 mK | -273 dB(WHz-1) | -184 dBW | -121 dB(Wm-2) | -222 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 123 - 126 GHz is used by the Radio Astronomy Service in:
Sharing problems with the following services:
Out-of-band emission from the following services: