Goto Section: 25.225 | 25.227 | Table of Contents
FCC 25.226
Revised as of October 1, 2016
Goto Year:2015 |
2017
§ 25.226 Blanket licensing provisions for domestic, U.S. VMESs operating
with GSO FSS space stations in the 10.95-11.2 GHz, 11.45-11.7 GHz, 11.7-12.2
GHz, and 14.0-14.5 GHz bands.
(a) The following ongoing requirements govern all VMES licensees and
operations in the 10.95-11.2 GHz (space-to-Earth), 11.45-11.7 GHz
(space-to-Earth), 11.7-12.2 GHz (space-to-Earth) and 14.0-14.5 GHz
(Earth-to-space) bands receiving from and transmitting to geostationary
orbit satellites in the Fixed-Satellite Service. VMES licensees shall
comply with the requirements in either paragraph (a)(1), (a)(2) or
(a)(3) of this section and all of the requirements set forth in
paragraphs (a)(4) through (a)(9) and paragraphs (c), (d), and (e) of
this section. Paragraph (b) of this section identifies items that shall
be included in the application for VMES operations to demonstrate that
these ongoing requirements will be met.
(1) The following requirements shall apply to a VMES that uses
transmitters with off-axis EIRP spectral-densities lower than or equal
to the levels in paragraph (a)(1)(i) of this section. A VMES, or VMES
system, operating under this section shall provide a detailed
demonstration as described in paragraph (b)(1) of this section. The
VMES transmitter also shall comply with the antenna pointing and
cessation of emission requirements in paragraphs (a)(1)(ii) and
(a)(1)(iii) of this section.
(i)(A) Off-axis EIRP spectral density emitted in the plane tangent to
the GSO arc, as defined in § 25.103, shall not exceed the following
values:
15-25logθ dBW/4 kHz for 1.5° ≤ θ ≤ 7°.
−6 dBW/4 kHz for 7° < θ ≤ 9.2°.
18-25logθ dBW/4 kHz for 9.2° < θ ≤ 19.1°.
−14 dBW/4 kHz for 19.1° < θ ≤ 180°.
Where theta (θ) is the angle in degrees from a line from the earth
station antenna to the assigned orbital location of the target
satellite. The EIRP density levels specified for θ > 7° may be exceeded
by up to 3 dB in up to 10% of the range of theta (θ) angles from
±7-180°, and by up to 6 dB in the region of main reflector spillover
energy.
(B) The off-axis EIRP spectral density of co-polarized signals shall
not exceed the following values in the plane perpendicular to the GSO
arc, as defined in § 25.103:
18-25logθ dBW/4 kHz for 3.0° ≤ θ ≤ 19.1°.
−14 dBW/4 kHz for 19.1° < θ ≤ 180°.
Where θ is as defined in paragraph (a)(1)(i)(A) of this section. These
EIRP density levels may be exceeded by up to 6 dB in the region of main
reflector spillover energy and in up to 10% of the range of θ angles
not included in that region, on each side of the line from the earth
station to the target satellite.
(C) The EIRP density of cross-polarized signals shall not exceed the
following values in the plane tangent to the GSO arc or in the plane
perpendicular to the GSO arc:
5-25logθ dBW/4 kHz for 1.8° ≤ θ ≤ 7.0°.
Where θ is as defined in paragraph (a)(1)(i)(A) of this section.
(ii) Except for VMES systems operating under paragraph (a)(3), each
VMES transmitter must meet one of the following antenna pointing error
requirements:
(A) Each VMES transmitter shall maintain a pointing error of less than
or equal to 0.2° between the orbital location of the target satellite
and the axis of the main lobe of the VMES antenna, or
(B) Each VMES transmitter shall declare a maximum antenna pointing
error that may be greater than 0.2° provided that the VMES does not
exceed the off-axis EIRP spectral-density limits in paragraph (a)(1)(i)
of this section, taking into account the antenna pointing error.
(iii) Except for VMES systems operating under paragraph (a)(3), each
VMES transmitter must meet of one the following cessation of emission
requirements:
(A) For VMESs operating under paragraph (a)(1)(ii)(A) of this section,
all emissions from the VMES shall automatically cease within 100
milliseconds if the angle between the orbital location of the target
satellite and the axis of the main lobe of the VMES antenna exceeds
0.5°, and transmission shall not resume until such angle is less than
or equal to 0.2°, or
(B) For VMES transmitters operating under paragraph (a)(1)(ii)(B) of
this section, all emissions from the VMES shall automatically cease
within 100 milliseconds if the angle between the orbital location of
the target satellite and the axis of the main lobe of the VMES antenna
exceeds the declared maximum antenna pointing error and shall not
resume transmissions until such angle is less than or equal to the
declared maximum antenna pointing error.
(2) The following requirements apply to VMES systems that operate with
off-axis EIRP spectral-densities in excess of the levels in paragraph
(a)(1)(i) or (a)(3)(i) of this section under licenses granted based on
certifications filed pursuant to paragraph (b)(2) of this section.
(i) A VMES or VMES system licensed based on certifications filed
pursuant to paragraph (b)(2) of this section must operate in accordance
with the off-axis EIRP density specifications provided to the target
satellite operator in order to obtain the certifications.
(ii) Any VMES transmitter operating under a license granted based on
certifications filed pursuant to paragraph (b)(2) of this section must
be self-monitoring and capable of shutting itself off and must cease or
reduce emissions within 100 milliseconds after generating off-axis
EIRP-density in excess of the specifications supplied to the target
satellite operator.
(iii) A system with variable power control of individual VMES
transmitters must monitor the aggregate off-axis EIRP density from
simultaneously transmitting VMES transmitters at the system's network
control and monitoring center. If simultaneous operation of two or more
VMES transmitters causes aggregate off-axis EIRP density to exceed the
off-axis EIRP density specifications supplied to the target satellite
operator, the network control and monitoring center must command those
transmitters to cease emissions or reduce the aggregate EIRP density to
a level at or below those specifications and the transmitters must
comply within 100 milliseconds of receiving the command.
(3) The following requirements apply to a VMES system that uses
variable power control of individual VMES earth stations transmitting
simultaneously in the same frequencies to the same target satellite,
unless the system operates pursuant to paragraph (a)(2) of this
section.
(i) Aggregate EIRP density from co-frequency earth stations in each
target satellite receiving beam, not resulting from colliding data
bursts transmitted pursuant to a contention protocol, will not exceed
the limits defined in paragraph (a)(1)(i) of this section.
(ii) Each VMES transmitter must be self-monitoring and capable of
shutting itself off and must cease or reduce emissions within 100
milliseconds after generating off-axis EIRP density in excess of the
limit in paragraph (a)(3)(i) of this section.
(iii) Aggregate power density from simultaneously transmitting VMES
transmitters must be monitored at the system's network control and
monitoring center. If simultaneous operation of two or more
transmitters in a VMES network causes aggregate off-axis EIRP density
to exceed the off-axis EIRP density limit in paragraph (a)(3)(i) of
this section, the network control and monitoring center must command
those transmitters to cease emissions or reduce the aggregate EIRP
density to a level at or below that limit, and those transmitters must
comply within 100 milliseconds of receiving the command.
(4) An applicant filing to operate a VMES terminal or system and
planning to use a contention protocol shall certify that its contention
protocol use will be reasonable.
(5) There shall be a point of contact in the United States, with phone
number and address, available 24 hours a day, seven days a week, with
authority and ability to cease all emissions from the VMESs.
(6) For each VMES transmitter, a record of the vehicle location (i.e.,
latitude/longitude), transmit frequency, channel bandwidth and
satellite used shall be time annotated and maintained for a period of
not less than one (1) year. Records shall be recorded at time intervals
no greater than every five (5) minutes while the VMES is transmitting.
The VMES operator shall make this data available upon request to a
coordinator, fixed system operator, Fixed-Satellite Service system
operator, NTIA, or the Commission within 24 hours of the request.
(7) In the 10.95-11.2 GHz (space-to-Earth) and 11.45-11.7 GHz
(space-to-Earth) frequency bands VMESs shall not claim protection from
interference from any authorized terrestrial stations to which
frequencies are either already assigned, or may be assigned in the
future.
(8) A VMES terminal receiving in the 10.95-11.2 GHz (space-to-Earth),
11.45-11.7 GHz (space-to-Earth) and 11.7-12.2 GHz (space-to-Earth)
bands shall receive protection from interference caused by space
stations other than the target space station only to the degree to
which harmful interference would not be expected to be caused to an
earth station employing an antenna conforming to the referenced
patterns defined in § 25.209(a) and (b) and stationary at the location
at which any interference occurred.
(9) Each VMES terminal shall automatically cease transmitting upon the
loss of synchronization or within 5 seconds upon loss of reception of
the satellite downlink signal, whichever is the shorter timeframe.
(b) Applications for VMES operation in the 14.0-14.5 GHz
(Earth-to-space) band to GSO satellites in the FSS must include, in
addition to the particulars of operation identified on FCC Form 312,
and associated Schedule B, applicable technical demonstrations pursuant
to paragraph (b)(1), (b)(2), or (b)(3) of this section and the
documentation identified in paragraphs (b)(4) through (b)(8) of this
section.
(1) A VMES applicant proposing to implement a transmitter under
paragraph (a)(1) of this section must provide the information required
by § 25.115(g)(1). An applicant proposing to implement a transmitter
under paragraph (a)(1)(ii)(A) of this section must also provide the
certifications identified in paragraph (b)(1)(iii) of this section. An
applicant proposing to implement a transmitter under paragraph
(a)(1)(ii)(B) of this section must also provide the demonstrations
identified in paragraph (b)(1)(iv) of this section.
(i)-(ii) [Reserved]
(iii) A VMES applicant proposing to implement a transmitter under
paragraph (a)(1)(ii)(A) of this section shall provide a certification
from the equipment manufacturer stating that the antenna tracking
system will maintain a pointing error of less than or equal to 0.2°
between the orbital location of the target satellite and the axis of
the main lobe of the VMES antenna and that the antenna tracking system
is capable of ceasing emissions within 100 milliseconds if the angle
between the orbital location of the target satellite and the axis of
the main lobe of the VMES antenna exceeds 0.5°.
(iv) A VMES applicant proposing to implement a transmitter under
paragraph (a)(1)(ii)(B) of this section shall:
(A) Declare, in its application, a maximum antenna pointing error and
demonstrate that the maximum antenna pointing error can be achieved
without exceeding the off-axis EIRP spectral-density limits in
paragraph (a)(1)(i) of this section; and
(B) Demonstrate that the VMES transmitter can detect if the transmitter
exceeds the declared maximum antenna pointing error and can cease
transmission within 100 milliseconds if the angle between the orbital
location of the target satellite and the axis of the main lobe of the
VMES antenna exceeds the declared maximum antenna pointing error, and
will not resume transmissions until the angle between the orbital
location of the target satellite and the axis of the main lobe of the
VMES antenna is less than or equal to the declared maximum antenna
pointing error.
(2) An applicant proposing to operate with off-axis EIRP density in
excess of the levels in paragraph (a)(1)(i) or (a)(3)(i) of this
section must provide the following in exhibits to its earth station
application:
(i) Off-axis EIRP density data pursuant to § 25.115(g)(1);
(ii) The certifications required by § 25.220(d);
(iii) A detailed showing that each VMES transmitter in the system will
automatically cease or reduce emissions within 100 milliseconds after
generating EIRP density exceeding specifications provided to the target
satellite operator; and
(iv) A detailed showing that the aggregate power density from
simultaneously transmitting VMES transmitters will be monitored at the
system's network control and monitoring center; that if simultaneous
operation of two or more VMES transmitters causes the aggregate
off-axis EIRP density to exceed the off-axis EIRP density
specifications supplied to the target satellite operator, the network
control and monitoring center will command those transmitters to cease
emissions or reduce the aggregate EIRP density to a level at or below
those specifications; and that those transmitters will comply within
100 milliseconds of receiving the command.
(3) An applicant proposing to implement a VMES system subject to
paragraph (a)(3) of this section must provide the following information
in exhibits to its earth station application:
(i) Off-axis EIRP density data pursuant to § 25.115(g)(1);
(ii) A detailed showing of the measures that will be employed to
maintain aggregate EIRP density at or below the limit in paragraph
(a)(3)(i) of this section;
(iii) A detailed showing that each VMES terminal will automatically
cease or reduce emissions within 100 milliseconds after generating
off-axis EIRP density exceeding the limit in paragraph (a)(3)(i) of
this section; and
(iv) A detailed showing that the aggregate power density from
simultaneously transmitting ESV transmitters will be monitored at the
system's network control and monitoring center; that if simultaneous
operation of two or more transmitters in the VMES network causes
aggregate off-axis EIRP density to exceed the off-axis EIRP density
limit in paragraph (a)(3)(i) of this section, the network control and
monitoring center will command those transmitters to cease emissions or
reduce the aggregate EIRP density to a level at or below that limit;
and that those transmitters will comply within 100 milliseconds of
receiving the command.
(4) There shall be an exhibit included with the application describing
the geographic area(s) in which the VMESs will operate.
(5) Any VMES applicant filing for a VMES terminal or system and
planning to use a contention protocol shall include in its application
a certification that will comply with the requirements of paragraph
(a)(4) of this section.
(6) The point of contact referred to in paragraph (a)(5) of this
section shall be included in the application.
(7) Any VMES applicant filing for a VMES terminal or system shall
include in its application a certification that will comply with the
requirements of paragraph (a)(6) of this section.
(8) All VMES applicants shall submit a radio frequency hazard analysis
determining via calculation, simulation, or field measurement whether
VMES terminals, or classes of terminals, will produce power densities
that will exceed the Commission's radio frequency exposure criteria.
VMES applicants with VMES terminals that will exceed the guidelines in
§ 1.1310 of this chapter for radio frequency radiation exposure shall
provide, with their environmental assessment, a plan for mitigation of
radiation exposure to the extent required to meet those guidelines. All
VMES licensees shall ensure installation of VMES terminals on vehicles
by qualified installers who have an understanding of the antenna's
radiation environment and the measures best suited to maximize
protection of the general public and persons operating the vehicle and
equipment. A VMES terminal exhibiting radiation exposure levels
exceeding 1.0 mW/cm2 in accessible areas, such as at the exterior
surface of the radome, shall have a label attached to the surface of
the terminal warning about the radiation hazard and shall include
thereon a diagram showing the regions around the terminal where the
radiation levels could exceed 1.0 mW/cm2. All VMES applicants shall
demonstrate that their VMES terminals are capable of automatically
ceasing transmissions upon the loss of synchronization or within 5
seconds upon loss of reception of the satellite downlink signal,
whichever is the shorter timeframe.
(9) Except for VMES systems operating pursuant to paragraphs (a)(2) and
(a)(3)(ii) of this section, VMES systems authorized pursuant to this
section shall be eligible for a license that lists Permitted List as an
authorized point of communication.
(c)(1) Operations of VMESs in the 14.0-14.2 GHz (Earth-to-space)
frequency band within 125 km of the NASA TDRSS facilities on Guam
(latitude 13°36′55″ N, longitude 144°51′22″ E) or White Sands, New
Mexico (latitude 32°20′59″ N, longitude 106°36′31″ W and latitude
32°32′40″ N, longitude 106°36′48″ W) are subject to coordination with
the National Aeronautics and Space Administration (NASA) through the
National Telecommunications and Information Administration (NTIA)
Interdepartment Radio Advisory Committee (IRAC). Licensees shall notify
the International Bureau once they have completed coordination. Upon
receipt of such notification from a licensee, the International Bureau
will issue a public notice stating that the licensee may commence
operations within the coordination zone in 30 days if no party has
opposed the operations.
(2) When NTIA seeks to provide similar protection to future TDRSS sites
that have been coordinated through the IRAC Frequency Assignment
Subcommittee process, NTIA will notify the Commission's International
Bureau that the site is nearing operational status. Upon public notice
from the International Bureau, all Ku-band VMES licensees shall cease
operations in the 14.0-14.2 GHz band within 125 km of the new TDRSS
site until the licensees complete coordination with NTIA/IRAC for the
new TDRSS facility. Licensees shall notify the International Bureau
once they have completed coordination for the new TDRSS site. Upon
receipt of such notification from a licensee, the International Bureau
will issue a public notice stating that the licensee may commence
operations within the coordination zone in 30 days if no party has
opposed the operations. The VMES licensee then will be permitted to
commence operations in the 14.0-14.2 GHz band within 125 km of the new
TDRSS site, subject to any operational constraints developed in the
coordination process.
(d)(1) Operations of VMESs in the 14.47-14.5 GHz (Earth-to-space)
frequency band in the vicinity of radio astronomy service (RAS)
observatories observing in the 14.47-14.5 GHz band are subject to
coordination with the National Science Foundation (NSF). The
appropriate NSF contact point to initiate coordination is
Electromagnetic Spectrum Manager, NSF, 4201 Wilson Blvd., Suite 1045,
Arlington VA 22203, fax 703-292-9034, e-mail esm@nsf.gov. Licensees
shall notify the International Bureau once they have completed
coordination. Upon receipt of the coordination agreement from a
licensee, the International Bureau will issue a public notice stating
that the licensee may commence operations within the coordination zone
in 30 days if no party has opposed the operations.
(2) Table 1 provides a list of each applicable RAS site, its location,
and the applicable coordination zone.
Table 1—Applicable Radio Astronomy Service (RAS) Facilities and
Associated Coordination Distances
Observatory Latitude (north) Longitude (west) Radius (km) of
coordination zone
Arecibo, Observatory, Arecibo, PR 18°20′37″ 66°45′11″ Island of Puerto
Rico.
Green Bank, WV 38°25′59″ 79°50′23″ 160.
Very Large Array, near Socorro, NM 34°04′44″ 107°37′06″ 160.
Pisgah Astronomical Research Institute, Rosman, NC 35°11′59″ 82°52′19″
160.
U of Michigan Radio Astronomy Observatory, Stinchfield Woods, MI
42°23′56″ 83°56′11″ 160.
Very Long Baseline Array (VLBA) stations:
Owens Valley, CA 37°13′54″ 118°16′37″ 160*.
Mauna Kea, HI 19°48′05″ 155°27′20″ 50.
Brewster, WA 48°07′52″ 119°41′00″
Kitt Peak, AZ 31°57′23″ 111°36′45″
Pie Town, NM 34°18′04″ 108°07′09″
Los Alamos, NM 35°46′30″ 106°14′44″
Fort Davis, TX 30°38′06″ 103°56′41″
North Liberty, IA 41°46′17″ 91°34′27″
Hancock, NH 42°56′01″ 71°59′12″
St. Croix, VI 17°45′24″ 64°35′01″
*Owens Valley, CA operates both a VLBA station and single-dish
telescopes.
(3) When NTIA seeks to provide similar protection to future RAS sites
that have been coordinated through the IRAC Frequency Assignment
Subcommittee process, NTIA will notify the Commission's International
Bureau that the site is nearing operational status. Upon public notice
from the International Bureau, all Ku-band VMES licensees shall cease
operations in the 14.47-14.5 GHz band within the relevant geographic
zone (160 kms for single-dish radio observatories and Very Large Array
antenna systems and 50 kms for Very Long Baseline Array antenna
systems) of the new RAS site until the licensees complete coordination
for the new RAS facility. Licensees shall notify the International
Bureau once they have completed coordination for the new RAS site and
shall submit the coordination agreement to the Commission. Upon receipt
of such notification from a licensee, the International Bureau will
issue a public notice stating that the licensee may commence operations
within the coordination zone in 30 days if no party opposed the
operations. The VMES licensee then will be permitted to commence
operations in the 14.47-14.5 GHz band within the relevant coordination
distance around the new RAS site, subject to any operational
constraints developed in the coordination process.
(e) VMES licensees shall use Global Positioning Satellite-related or
other similar position location technology to ensure compliance with
paragraphs (c) and (d) of this section.
[ 74 FR 57099 , Nov. 4, 2009, as amended at 78 FR 8429 , Feb. 6, 2013; 78 FR 9604 , Feb. 11, 2013; 79 FR 8324 , Feb. 12, 2014; 81 FR 55345 , Aug.
18, 2016]
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Goto Section: 25.225 | 25.227
Goto Year: 2015 |
2017
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