FCC 25.213 Revised as of October 1, 2005
Goto Year:2004 |
2006
Sec. 25.213 Inter-Service coordination requirements for the 1.6/2.4 GHz
mobile-satellite service.
(a) Protection of the radio astronomy service in the 1610.6–1613.8 MHz band
against interference from 1.6/2.4 GHz Mobile-Satellite Service systems.
(1) Protection zones. All 1.6/2.4 GHz Mobile Satellite Service systems shall
be capable of determining the position of the user transceivers accessing
the space segment through either internal radiodetermination calculations or
external sources such as LORAN-C or the Global Positioning System. During
periods of radio astronomy observations, land mobile earth stations shall
not operate when located within geographic protection zones defined by the
radio observatory coordinates and separation distances as follows:
(i) In the band 1610.6–1613.8 MHz, within a 160 km radius of the following
radio astronomy sites:
------------------------------------------------------------------------
Latitude Longitude
Observatory (DMS) (DMS)
------------------------------------------------------------------------
Arecibo, PR..................................... 18 20 46 66 45 11
Green Bank Telescope, WV........................ 38 25 59 79 50 24
38 26 09 79 49 42
Very Large Array, NM............................ 34 04 43 107 37 04
Owens Valley, CA................................ 37 13 54 118 17 36
Ohio State, OH.................................. 40 15 06 83 02 54
------------------------------------------------------------------------
(ii) In the band 1610.6–1613.8 MHz, within a 50 km radius of the following
sites:
------------------------------------------------------------------------
Latitude Longitude
Observatory (DMS) (DMS)
------------------------------------------------------------------------
Pile Town, NM................................... 34 18 04 108 07 07
Los Alamos, NM.................................. 35 46 30 106 14 42
Kitt Peak, AZ................................... 31 57 22 111 36 42
Ft. Davis, TX................................... 30 38 06 103 56 39
N. Liberty, IA.................................. 41 46 17 91 34 26
Brewster, WA.................................... 48 07 53 119 40 55
Owens Valley, CA................................ 37 13 54 118 16 34
St. Croix, VI................................... 17 45 31 64 35 03
Mauna Kea, HI................................... 19 48 16 155 27 29
Hancock, NH..................................... 42 56 01 71 59 12
------------------------------------------------------------------------
(iii) Out-of-band emissions of a mobile earth station licensed to operate
within the 1610.0–1626.5 MHz band shall be attenuated so that the power flux
density it produces in the 1610.6–1613.8 MHz band at any radio astronomy
site listed in paragraph (a)(1) (i) or (ii) of this section shall not exceed
the emissions of a mobile earth station operating within the 1610.6–1613.8
MHz band at the edge of the protection zone applicable for that site. As an
alternative, a mobile earth station shall not operate during radio astronomy
observations within the 1613.8–1615.8 MHz band within 100 km of the radio
astronomy sites listed in paragraph (a)(1)(i) of this section, and within 30
km of the sites listed in paragraph (a)(1)(ii) of this section, there being
no restriction on a mobile earth station operating within the 1615.8–1626.5
MHz band.
(iv) For airborne mobile earth stations operating in the 1610.0–1626.5 MHz
band, the separation distance shall be the larger of the distances specified
in paragraph (a)(1) (i), (ii) or (iii) of this section, as applicable, or
the distance, d, as given by the formula:
d (km) = 4.1 square root of (h)
where h is the altitude of the aircraft in meters above ground level.
(v) Smaller geographic protection zones may be used in lieu of the areas
specified in paragraphs (a)(1) (i), (ii), (iii), and (iv) of this section if
agreed to by the Mobile-Satellite Service licensee and the Electromagnetic
Spectrum Management Unit (ESMU), National Science Foundation, Washington,
D.C. upon a showing by the Mobile-Satellite Service licensee that the
operation of a mobile earth station will not cause harmful interference to a
radio astronomy observatory during periods of observation.
(vi) The ESMU shall notify Mobile-Satellite Service space station licensees
authorized to operate mobile earth terminals in the 1610.0–1626.5 MHz band
of periods of radio astronomy observations. The mobile-satellite systems
shall be capable of terminating operations within the frequency bands and
protection zones specified in paragraphs (a)(1) (i) through (iv) of this
section, as applicable, after the first position fix of the mobile earth
terminal either prior to transmission or, based upon its location within the
protection zone at the time of initial transmission of the mobile earth
terminal. Once the mobile-satellite system determines that a mobile earth
terminal is located within an RAS protection zone, the mobile-satellite
system shall immediately initiate procedures to relocate the mobile earth
terminal operations to a non-RAS frequency.
(vii) A beacon-actuated protection zone may be used in lieu of fixed
protection zones in the 1610.6–1613.8 MHz band if a coordination agreement
is reached between a mobile-satellite system licensee and the ESMU on the
specifics of beacon operations.
(viii) Additional radio astronomy sites, not located within 100 miles of the
100 most populous urbanized areas as defined by the United States Census
Bureau at the time, may be afforded similar protection one year after notice
to the mobile-satellite system licensees by issuance of a public notice by
the Commission.
(2) Mobile-Satellite Service space stations transmitting in the
1613.8–1626.5 MHz band shall take whatever steps necessary to avoid causing
harmful interference to the radio astronomy facilities listed in paragraphs
(a)(1)(i) and (ii) of this section during periods of observation.
(3) Mobile-Satellite Service space stations operating in the 2483.5–2500 MHz
frequency band shall limit spurious emission levels in the 4990–5000 MHz
band so as not to exceed −241 dB (W/m^2/Hz) at the surface of the Earth.
(4) The Radioastronomy Service shall avoid scheduling radio astronomy
observations during peak MSS/RDSS traffic periods to the greatest extent
practicable.
(b) [Reserved]
[ 59 FR 53329 , Oct. 21, 1994, as amended at 61 FR 9945 , Mar. 12, 1996; 67 FR 61816 , Oct. 2, 2002]
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