U.S. Non-Federal-Government Allocations
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93.999999999 GHz (93,999,999,999 Hz)
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FIXED 5.338A
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FIXED 5.338A
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FIXED 5.338A
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5.149 In making assignments to stations of other services to which the bands:
13 360-13 410 kHz,
25 550-25 670 kHz,
37.5-38.25 MHz,
73-74.6 MHz in Regions 1 and 3,
150.05-153 MHz in Region 1,
322-328.6 MHz,
406.1-410 MHz,
608-614 MHz in Regions 1 and 3,
1 330-1 400 MHz,
1 610.6-1 613.8 MHz,
1 660-1 670 MHz,
1 718.8-1 722.2 MHz,
2 655-2 690 MHz,
3 260-3 267 MHz,
3 332-3 339 MHz,
3 345.8-3 352.5 MHz,
4 825-4 835 MHz, 4 950-4 990 MHz,
4 990-5 000 MHz,
6 650-6 675.2 MHz,
10.6-10.68 GHz,
14.47-14.5 GHz,
22.01-22.21 GHz,
22.21-22.5 GHz,
22.81-22.86 GHz,
23.07-23.12 GHz,
31.2-31.3 GHz,
31.5-31.8 GHz in Regions 1 and 3,
36.43-36.5 GHz,
42.5-43.5 GHz,
48.94-49.04 GHz,
76-86 GHz,
92-94 GHz,
94.1-100 GHz, 102-109.5 GHz,
111.8-114.25 GHz,
128.33-128.59 GHz,
129.23-129.49 GHz,
130-134 GHz,
136-148.5 GHz,
151.5-158.5 GHz,
168.59-168.93 GHz,
171.11-171.45 GHz,
172.31-172.65 GHz,
173.52-173.85 GHz,
195.75-196.15 GHz,
209-226 GHz,
241-250 GHz,
252-275 GHz
are allocated, administrations are urged to take all practicable steps 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 Nos. 4.5 and 4.6 and Article 29). (WRC 07)
5.338A In the frequency bands 1 350-1 400 MHz, 1 427-1 452 MHz, 22.55-23.55 GHz, 24.25-27.5 GHz, 30-31.3 GHz, 49.7 50.2 GHz, 50.4-50.9 GHz, 51.4-52.4 GHz, 52.4-52.6 GHz, 81-86 GHz and 92-94 GHz, Resolution 750 (Rev.WRC 19) applies. (WRC 19)
US161 In the bands 81-86 GHz, 92-94 GHz, and 94.1-95 GHz and within the coordination distances indicated below, assignments to allocated services shall be coordinated with the following radio astronomy observatories. New observatories shall not receive protection from fixed stations that are licensed to operate in the one hundred most populous urbanized areas as defined by the U.S. Census Bureau for the year 2000.
(a) Within 25 km of the National Radio Astronomy Observatory’s (NRAO’s) Very Long Baseline Array (VLBA) Stations:
| State | VLBA Station | Lat. (N) | Long. (W) |
| AZ | Kitt Peak | 31° 57` 23" | 111° 36` 45" |
| CA | Owens Valley | 37° 13` 54" | 118° 16` 37" |
| HI | Mauna Kea | 19° 48` 05" | 155° 27` 20" |
| IA | North Liberty | 41° 46` 17" | 091° 34` 27" |
| NH | Hancock | 42° 56` 01" | 071° 59` 12" |
| NM | Los Alamos | 35° 46` 30" | 106° 14` 44" |
| NM | Pie Town | 34° 18` 04" | 108° 07` 09" |
| TX | Fort Davis | 30° 38` 06" | 103° 56` 41" |
| VI | Saint Croix | 17° 45` 24" | 064° 35` 01" |
| WA | Brewster | 48° 07` 52" | 119° 41` 00" |
(b) Within 150 km of the following observatories:
| State | Telescope and site | Lat. (N) | Long. (W) |
| AZ | Heinrich Hertz Submillimeter Observatory, Mt. Graham | 32° 42` 06" | 109° 53` 28" |
| AZ | University of Arizona 12-m Telescope, Kitt Peak | 31° 57` 12" | 111° 36` 53" |
| CA | Caltech Telescope, Owens Valley | 37° 13` 54" | 118° 17` 36" |
| CA | Combined Array for Research in Millimeter-wave Astronomy (CARMA) | 37° 16` 43" | 118° 08` 32" |
| HI | James Clerk Maxwell Telescope, Mauna Kea | 19° 49` 33" | 155° 28` 47" |
| MA | Haystack Observatory, Westford | 42° 37` 24" | 071° 29` 18" |
| NM | NRAO’s Very Large Array, Socorro | 34° 04` 44" | 107° 37` 06" |
| WV | NRAO’s Robert C. Byrd Telescope, Green Bank | 38° 25` 59" | 079° 50` 23" |
Note: Satisfactory completion of the coordination procedure utilizing the automated mechanism, see 47 CFR 101.1523, will be deemed to establish sufficient separation from radio astronomy observatories, regardless of whether the distances set forth above are met.
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).