Representatives of Satellite System License, Inc., a wholly owned subsidiary of Motorola, Inc.,
("Motorola") under contract to Iridium LLC ("Iridium"), and the National Astronomy and
Ionosphere Center(1) ("NAIC") have carried out technical discussions pursuant to the
Framework Agreement between the parties, dated 19 March 1997. This Coordination Agreement
has been developed in accordance with the aforementioned Framework Agreement, and refers to
the applicable FCC regulations, and the Principles for Coordination contained therein.
2) FCC REGULATIONS
The FCC has established certain inter-service coordination requirements for satellite systems
operating in the 1610-1626.5 MHz band. These requirements are contained in Section 25.213 of
the FCC's Rules and Regulations. They include:
47 CFR 25.213(a)(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 [list of observatories, including
Arecibo Radio Observatory] during periods of observation.
47 CFR 25.213(a)(4):
The Radio Astronomy Service shall avoid scheduling radio astronomy observations during peak
MSS/RDSS traffic periods to the greatest extent practicable.
3) PRINCIPLES OF COORDINATION
The following basic principles have been agreed upon regarding the coordination of the
IRIDIUM(R) System(2) with the Arecibo Radio Astronomy Observatory ("Arecibo"):
a) Motorola/Iridium will operate the IRIDIUM System in a spectrum efficient and economic
manner, without causing harmful interference to Arecibo. It is recognized that the main area of
concern is potential interference to the radio astronomy observations scheduled at Arecibo in the
1610.6-1613.8 MHz band from the IRIDIUM System downlinks, covered by international RR
b) Arecibo is to be protected from harmful interference during those periods that radio astronomy
observations are conducted in the 1610.6-1613.8 MHz band. The scheduling of these periods will,
to the greatest extent practicable, be done in such a way as to coincide with the minimum traffic
periods for the IRIDIUM System. It is anticipated that observations at Arecibo will not
unnecessarily inhibit the ability of Motorola/Iridium to operate the IRIDIUM System in a
spectrum efficient and economic manner.
c) The IRIDIUM System mobile earth terminals will be capable of terminating operations after the
first position fix of the terminals.
d) The NAIC will provide Motorola/Iridium with scheduling information, either directly or
through the Electromagnetic Spectrum Management Unit of the National Science Foundation
(ESMU), regarding the periods when radio astronomy observations in the 1610.6-1613.8 MHz
band are expected to be conducted at Arecibo.
e) Motorola/Iridium will provide to the NAIC, at no charge, an air interface to the IRIDIUM
System that provides a signal with a blanking period during approximately 50% of each 90
millisecond time frame. This signal will indicate when the transmitters on board the IRIDIUM
System space vehicles are active. It is understood that the use of the air interface reduces the
sensitivity of the Arecibo telescope, and that it allows carrying out only some types of radio
astronomy observations. Nevertheless, it will enable NAIC, at its option, to conduct certain
observations at Arecibo at any time, by seeing through the IRIDIUM System transmissions.
f) The parties recognize that the provisions of this Coordination Agreement are based on the
unique conditions and facilities of Arecibo, and may not apply to Motorola/Iridium's coordination
with any other radio astronomy observatory in the U.S. or elsewhere.
Arecibo is a unique national facility that accepts observing proposals from scientists all over the
world. Observing time on the instrument is granted to projects reviewed favorably by external
referees, solely on the basis of scientific merit. Therefore, prior to the proposal deadline, Arecibo
can neither predict nor modify the total number of observing hours in any band during a particular
scheduling period; this is set by proposal pressure and the reviewers. Nothing in this
Coordination Agreement shall be construed as restricting or limiting Arecibo's ability to accept
and review proposals, and to grant observing time solely on the basis of scientific merit.
Except when lightly loaded, it is anticipated that the IRIDIUM System will produce an average
SPFD not exceeding -223 dBW m-2 Hz-1 in the 1610.6-1613.8 MHz band at the surface of the
Earth at Arecibo. This figure reflects the fact that IRIDIUM space vehicle antennas will transmit
in one polarization only, that the transmissions are averaged over a 2000 second interval, and that
the satellite is in the 0 dBi sidelobe of the Arecibo antenna.
Recommendation ITU-R RA.769, Table 2, provides detrimental interference threshold levels for
spectral line radio astronomy observations in the 1610.6-1613.8 MHz band as -238 dBW m-2
Hz-1 assuming, inter alia:
2000 second integration time and 20 kHz bandwidth for the radio astronomy observations;
interference is received through 0 dBi sidelobes of the radio telescope.
Coordination between the parties to this Coordination Agreement is based upon the following
a) Starting in 1999, Motorola/Iridium will provide quarterly to the NAIC the best available
information about the expected IRIDIUM System traffic patterns in the vicinity of Arecibo, in the
form of an hourly ranking for a typical week. NAIC will provide Motorola/Iridium with the best
available information about the scheduled observations in the 1610.6-1613.8 MHz band, a month
in advance of the observations. The parties will establish mutually convenient dates for the
exchange of this information.
b) Motorola/Iridium agrees to protect Arecibo to the SPFD level -238 dBW m-2 Hz-1 or better
from 10 p.m. to 6 a.m. (Miami local time) seven days a week during periods when observations
which have been notified to Motorola/Iridium in accordance with the procedure set forth in 4(a),
above, are being taken. These levels will be adjusted to reflect actual sidelobe performance of the
Arecibo antenna as determined by Arecibo and evaluated and jointly agreed upon by the parties.
c) A few observations of special celestial objects (comets, supernovae, and other celestial objects
of heretofore unknown type) may need to be accommodated outside the agreed 10 p.m.- 6 a.m.
scheduling window. To the greatest extent practicable, these observations will be carried out
using the blanker described in 3(e), above. Special observations that cannot be done using the
blanker will be protected to the -238 dBW m-2 Hz-1 level as set forth in 4(b), above. Such
observations shall not exceed 8 passes per calendar year.
d) Motorola/Iridium will comply with Section 25.213(a)(2) of the FCC's Rules as currently
formulated (see Section 2 herein) as applied to the Arecibo Observatory.
e) Motorola/Iridium will attempt to reduce emissions of any future generation satellites in the
IRIDIUM System into the 1610.6-1613.8 MHz band. The NAIC will continue to attempt to
decrease the Arecibo telescope's susceptibility to interference from spaceborne systems (e.g., by
reducing sidelobe levels, effects on the antenna pattern due to screen illumination, and by
incorporating blanking or other signal processing techniques into the observations).
5) PARTICIPATION IN TEST PROGRAM
Motorola agrees to allow representatives of the NAIC to participate in the scheduled
NRAO/Motorola radio astronomy test program, provided NRAO concurs. NAIC representatives
will also be allowed to review pertinent results of the testing subject to existing non-disclosure
The terms and provisions of this Coordination Agreement will not be held as confidential. Certain
information, to be exchanged under the terms of this agreement, and information that was
exchanged in the course of these negotiations, and was marked as Motorola Confidential
Proprietary, will remain confidential.
This Coordination Agreement may be modified only by mutual agreement, in writing. In the event
the parties reach an impasse on changes to this Coordination Agreement, they agree to submit the
issue to the FCC and NTIA for mediation and resolution.
The parties agree to work on the items listed in the Annex and to meet annually beginning in
February 1999 to review this Coordination Agreement.
ACCEPTED AND AGREED UPON:
It is understood that the undersigned have the actual authority necessary to bind their respective
companies and organizations to this Coordination Agreement.
This agreement may be executed by counterparts, each of which shall be deemed to be an original
but all of which together shall constitute one and the same instrument.
Dr. Paul E. Goldsmith
Director of Spectrum
Motorola Satellite Division,
James G. Ennis
Deputy General Counsel
1 March 1998
1. AREAS OF INVESTIGATION BY MOTOROLA
In accordance with the "Areas for Further Investigation" in the Framework Agreement dated 19
March 1997, and the associated Work Plan, Motorola has:
a) Provided preliminary information on expected 24-hour IRIDIUM System traffic patterns,
ranked hourly. No weekday/weekend data is currently available, but it is expected that such data
will become available as the system becomes operational.
b) Provided estimates of SPFD of a single IRIDIUM System burst transmission in the band
1610.6 - 1613.8 MHz, and the spectral signal characteristics of the IRIDIUM System within the
same band, as a function of loading.
c) Investigated the grouping of carriers to higher frequencies and local channel crowding, and
found that this approach will not reduce emissions into the band of interest to radio astronomy
under the current constraints on the IRIDIUM System. Channel crowding will be further
investigated in future generation IRIDIUM System satellites.
d) Conducted a study on the IRIDIUM System satellite elevation angle statistics at Arecibo. The study shows that, in relation to the Arecibo telescope, all IRIDIUM satellites are at off-axis angles of:
i) More than 48 degrees about 80% of the time;
ii) More than 30 degrees about 95% of the time;
iii) More than 19 degrees about 98% of the time.
e) Provided information on filters used during testing of the IRIDIUM System with National
Radio Astronomy Observatory, which reduce emissions from the IRIDIUM space vehicles in the
1621.35-1626.5 MHz band.
2. AREAS OF INVESTIGATION BY NAIC
In accordance with the "Areas of Further Investigation" in the aforementioned Framework
Agreement, and the associated Work Plan, NAIC has:
a) Determined, based on 1988 data, that:
i) Most Arecibo observations in the 1610.6 - 1613.8 MHz band could be scheduled between 8
p.m. and 6 a.m. local time every day of the week and one full day per week, e.g., Saturdays or
ii) A small number of observations (approximately 36 hours during the year) could not be fit into
such a schedule and require additional time.
b) Provided a study of bandwidth and integration time distribution, based on 1988 data, to show
that, relative to the -238 dBW m-2 Hz-1 detrimental interference level specified in ITU-R
i) 5% of the observations required 3-6 dB less sensitive measurements;
ii) 13% of the observations require 0-3 dB less sensitive measurements;
iii) 18% of the observations require 0-3 dB more sensitive measurements;
iv) 52% of the observations require 3-6 dB more sensitive measurements;
v) 12% of the observations require 6-9 dB more sensitive measurements.
c) Provided information on the current estimate of the Arecibo telescope's sidelobe structure.
d) Provided information showing that using simulations of dual beam switching techniques of the
Arecibo receivers reduced the effect of GLONASS interference to an acceptable level
approximately 70% of the time.
3. FUTURE AND ONGOING WORK
a) The NAIC will, as soon as practicable, measure the actual Arecibo antenna sidelobe
characteristics. NAIC will promptly provide a copy of the results to Motorola/Iridium.
b) Motorola/NAIC will evaluate the effect of interference from the IRIDIUM System using
techniques similar to those employed in 2(d) of this Annex.
c) The parties agree to jointly evaluate new data and techniques which may affect this Agreement.
This evaluation includes, but is not limited to, data regarding actual traffic loads and actual
demand for observing time; test results of the levels of interference generated by the IRIDIUM
System; averaging techniques that would ameliorate interference from the IRIDIUM System; and
improvements to the Arecibo antenna's sidelobes.
(1) The National Astronomy and Ionosphere Center is operated by Cornell University, under a
Cooperative Agreement with the National Science Foundation.
(2) IRIDIUM is a registered trademark and service mark of Iridium LLC.
Reinaldo Velez (10/10/2000)