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GLOBALSTAR and Boeing Coordination

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When an airborne mobile Earth station is within 4.1( h) km (where h is the ... and other celestial objects of heretofore unknown type) that are not anticipated ... – PowerPoint PPT presentation

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Title: GLOBALSTAR and Boeing Coordination


1
GLOBALSTAR and BoeingCoordination
  • T. Gergely
  • Summer School on Spectrum
  • Management and Radio Astronomy
  • Green Bank, June 2002

2
Globalstar Coordination-1
  • OH observations the band 1610.6-1613.8 MHz made
    at the NRAO sites and Arecibo.
  • Globalstar, L.P. operates a mobile satellite
    communications system in the 1610-1621.35 MHz
    band.
  • The agreement intends to facilitate sharing the
    band by Radio Astronomy observatories and
    Globalstar network uplinks from airplanes to
    satellites.

3
Globalstar Coordination -2
  • Globalstar obligations
  • When an airborne mobile Earth station is within
    4.1(? h) km (where h is the aircraft altitude in
    meters) of a radio astronomy site that is making
    observations, the average unwanted emission
    levels at the input port to the transmit antenna
    for any 1 MHz segment in the band 1610.6 - 1613.8
    MHz from the airborne mobile Earth station shall
    not exceed -65 dBW/MHz, with a corresponding
    aircraft underside antenna gain of nominally -10
    dBi or lower gain.
  • When an airborne mobile Earth station is within
    4.1(? h) km of a radio astronomy site that is not
    making observations, any licensed Globalstar
    frequency may be used.
  • NSF/ Radio astronomers Obligations
  • Provide an observation schedule for the band
    1610.6 - 1613.8 MHz for the sites included in the
    MoU, with two weeks advance notice

4
Globalstar CoordinationTimeline
  • Nov, 2000 GLOBALSTAR approaches NSF to coordinate
    airborne phone terminals and Proposes maximum
    unwanted emission levels in the 1612 and 1660
    MHz bands
  • Jan, 2001 Radio astronomy group (NRAO, NAIC, NSF
    and others) meets with GLOBALSTAR engineers,
    considers and rejects proposal as inadequate.
  • March, 2001 GLOBALSTAR simulations, based on
    improved unwanted emission characteristics show
    that new standards protect radio observatories
    from interference, except for 1 hr/day (at all
    US observatories)
  • April, 2001 Radio astronomy group decides to
    work on an agreement based on this simulation
  • Nov., 2001 Agreement between GLOBALSTAR and NSF
    signed
  • Observatories protected during periods of
    observations, except 1 hr. daily (peak GLOBALSTAR
    traffic)
  • Radio Observatories must notify GLOBALSTAR of
    their schedules
  • Jan - Feb, 2001 GLOBALSTAR declares Ch. 11

5
Boeing (Connexion) Coordination - 1
  • The 14.47-14.5 GHz band is allocated to radio
    astronomy on a secondary basis for observations
    of the formaldehyde (H2CO) line.
  • The 14.0 - 14.5 GHz band is allocated to the
    mobile-satellite (except aeronautical
    mobile-satellite) service (Earth-to-space) on a
    secondary basis.
  • Boeing filed an application with the FCC for
    authority to operate up to eight hundred
    technically identical transmit/receive mobile
    earth stations aboard aircraft to operate in the
    11.7 12.2 ? and 14.0 14.5 GHz ? bands.
  • US proposal to remove the restriction placed on
    the aeronautical mobile-satellite service
    (Earth-to-space) at WRC-03,

6
Boeing (Connexion) Coordination - 2
  • Boeing will
  • Cease AES transmissions in the 14.47 - 14.5 GHz
    band, within line-of sight of radio astronomy
    stations listed in Section 2.1, during periods of
    notified radio astronomy observations at the
    site.
  • Control the AES transmitters so that the pfd
    levels in the 14.47 14.5 GHz band produced at
    radio astronomy sites by individual AESs, during
    notified periods of observation (see Section
    3.7), does not exceed
  • pfd ?182 0.5? for ? lt 10
  • pfd ?177 for 10 lt ? lt 90
  • ? is the angle of arrival, measured in
    degrees, the pfd is expressed in units of
    dB(W/m2/MHz). (met by reducing power, ceasing
    transmissions, or changing frequencies of AESs
    that would exceed the pfd criteria)
  • Respond, as expeditiously as practicable, to an
    NSF request for protection of any site , for
    observations of special transient celestial
    objects (comets, supernovae, and other celestial
    objects of heretofore unknown type) that are not
    anticipated by the schedule of Section 3.7, and
    that may need to be accommodated on shorter
    notice. Requests for such observations are not
    expected to exceed 40 hours per calendar year.

7
Boeing (Connexion) Coordination - 3
  • NSF will
  • Maintain an observation schedule for the band
    14.47 - 14.5 GHz for the sites listed in Section
    2.1 and provide this schedule via both e-mail and
    fax, to the designated CBB point-of-contact
    address listed in Section 5.2 at least one week
    prior to the scheduled observations.
  • Provide, through NAIC and NRAO full access to
    CBB representatives to data on interference that
    may be collected during observations that fall
    within the scope of this agreement.
  • Coordination agreement signed December, 2001
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