SpectrumWiki
Radio spectrum allocations
Look up a frequency or a range.
Examples: 88.5 MHz, 1350–1430 MHz, 2.4 GHz
4.799999999 GHz (4,799,999,999 Hz)
U.S. Federal Government Allocations
FIXED
MOBILE
ITU Region 1 Allocations
FIXED
FIXED-SATELLITE (space-to-Earth) 5.441
MOBILE 5.440A
ITU Region 2 Allocations
FIXED
FIXED-SATELLITE (space-to-Earth) 5.441
MOBILE 5.440A
ITU Region 3 Allocations
FIXED
FIXED-SATELLITE (space-to-Earth) 5.441
MOBILE 5.440A
Footnotes
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5.440A In Region 2 (except Brazil, Cuba, French overseas departments and communities, Guatemala, Paraguay, Uruguay and Venezuela), and in Australia, the band 4 400-4 940 MHz may be used for aeronautical mobile telemetry for flight testing by aircraft stations (see No. 1.83). Such use shall be in accordance with Resolution 416 (WRC 07) and shall not cause harmful interference to, nor claim protection from, the fixed-satellite and fixed services. Any such use does not preclude the use of this band by other mobile service applications or by other services to which this band is allocated on a co-primary basis and does not establish priority in the Radio Regulations. (WRC-07)
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5.441 The use of the bands 4 500-4 800 MHz (space-to-Earth), 6 725-7 025 MHz (Earth-to-space) by the fixed-satellite service shall be in accordance with the provisions of Appendix 30B. The use of the bands 10.7-10.95 GHz (space-to-Earth), 11.2-11.45 GHz (space-to-Earth) and 12.75-13.25 GHz (Earth-to-space) by geostationary-satellite systems in the fixed-satellite service shall be in accordance with the provisions of Appendix 30B. The use of the bands 10.7-10.95 GHz (space-to-Earth), 11.2-11.45 GHz (space-to-Earth) and 12.75-13.25 GHz (Earth-to-space) by a non geostationary-satellite system in the fixed-satellite service is subject to application of the provisions of No. 9.12 for coordination with other non-geostationary-satellite systems in the fixed-satellite service. Non geostationary-satellite systems in the fixed-satellite service shall not claim protection from geostationary-satellite networks in the fixed-satellite service operating in accordance with the Radio Regulations, irrespective of the dates of receipt by the Bureau of the complete coordination or notification information, as appropriate, for the non-geostationary-satellite systems in the fixed-satellite service and of the complete coordination or notification information, as appropriate, for the geostationary-satellite networks, and No. 5.43A does not apply. Non-geostationary-satellite systems in the fixed-satellite service in the above bands shall be operated in such a way that any unacceptable interference that may occur during their operation shall be rapidly eliminated. (WRC 2000)
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US113 Radio astronomy observations of the formaldehyde line frequencies 4825-4835 MHz and 14.47-14.5 GHz may be made at certain radio astronomy observatories as indicated below:
Bands to be Observed 4 GHz 14 GHz Observatory X National Astronomy and Ionosphere Center (NAIC), Arecibo, PR X X National Radio Astronomy Observatory (NRAO), Green Bank, WV X X NRAO, Socorro, NM X Allen Telescope Array (ATA), Hat Creek, CA X X Owens Valley Radio Observatory (OVRO), Big Pine, CA X X NRAO's ten Very Long Baseline Array (VLBA) stations (see US131) X X University of Michigan Radio Astronomy Observatory, Stinchfield Woods, MI X Pisgah Astronomical Research Institute, Rosman, NC Every practicable effort will be made to avoid the assignment of frequencies to stations in the fixed or mobile services in these bands. Should such assignments result in harmful interference to these observations, the situation will be remedied to the extent practicable.
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US245 In the bands 3600-3650 MHz (space-to-Earth), 4500-4800 MHz (space-to-Earth), and 5850-5925 MHz (Earth-to-space), the use of the non-Federal fixed-satellite service is limited to international inter-continental systems and is subject to case-by-case electromagnetic compatibility analysis. The FCC's policy for these bands is codified at 47 CFR 2.108.
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US342 In making assignments to stations of other services to which the bands:
13 360-13 410 kHz 42.77-42.87 GHz* 25 550-25 670 kHz 43.07-43.17 GHz* 37.5-38.25 MHz 43.37-43.47 GHz* 322-328.6 MHz* 48.94-49.04 GHz* 1330-1400 MHz* 76-86 GHz 1610.6-1613.8 MHz* 92-94 GHz 1660-1660.5 MHz* 94.1-100 GHz 1668.4-1670 MHz* 102-109.5 GHz 3260-3267 MHz* 111.8-114.25 GHz 3332-3339 MHz* 128.33-128.59 GHz* 3345.8-3352.5 MHz* 129.23-129.49 GHz* 4825-4835 MHz* 130-134 GHz 4950-4990 MHz 136-148.5 GHz 6650-6675.2 MHz* 151.5-158.5 GHz 14.47-14.5 GHz* 168.59-168.93 GHz* 22.01-22.21 GHz* 171.11-171.45 GHz* 22.21-22.5 GHz 172.31-172.65 GHz* 22.81-22.86 GHz* 173.52-173.85 GHz* 23.07-23.12 GHz* 195.75-196.15 GHz* 31.2-31.3 GHz 209-226 GHz 36.43-36.5 GHz* 241-250 GHz 42.5-43.5 GHz 252-275 GHz are allocated (*indicates radio astronomy use for spectral line observations), all practicable steps shall be taken to protect the radio astronomy service from harmful interference. Emissions from spaceborne or airborne stations can be particularly serious sources of interference to the radio astronomy service (see ITU Radio Regulations at Nos. 4.5 and 4.6 and Article 29).