NSF agreement

0026-EX-ST-2013 Text Documents

Panasonic Avionics Corporation

2013-03-28ELS_135037

COORDINATION AGREEMENT FOR THE JOINT USAGE OF THE
  BAND 14.0 - 14.5 GHz BETWEEN THE NATIONAL SCIENCE
 FOUNDATION AND PANASONIC AVIONICS CORPORATION




                      Version 1.1




                   December 18, 2009


                            Coordination Agreement for the Joint Usage
                         of the Band 14.0 - 14.5 GHz Between the National
                     Science Foundation and Panasonic Avionics Corporation


Panasonic Avionics Corporation (PAC) is applying for authority to operate a global Aeronautical
Mobile-Satellite Service (AMSS) network in the 14.0-14.5 GHz Fixed-Satellite Service (FSS)
band. The AMSS terminals will be installed aboard commercial aircraft and operate with
commercial geostationary satellites. This coordination agreement and the pending Federal
Communications Commission (FCC) license comply with FCC Part 25 rules and the
recommendations of the International Telecommunication Union (ITU) as a product of the
World Radiocommunication Conference WRC-03.

1.     Overview

       1.1    The band 14.47-14.5 GHz is used by the radio astronomy service in accordance
              with footnotes US342 to the U.S. Table of Frequency Allocations

       1.2    The band 14.0-14.5 GHz has been allocated to mobile-satellite service including
              AMSS on a secondary basis with the provision that government services,
              including the radio astronomy service in the 14.47-14.50 GHz band, be protected
              from interference from the AMSS service.

       1.3    PAC filed an application with the FCC on July 24, 2009 for experimental
              authority to operate two types of transmit/receive aircraft earth stations (AES) and
              also plans to submit a commercial license application to the FCC.

       1.4    The AMSS operations will allow AESs to transmit and receive information from a
              ground earth station via a transponder on geostationary satellites arc under the
              control of a ground-based network operation center in Miramar, FL.

       1.5    This Coordination Agreement ensures that the PAC AMSS system complies with
              both Part 25 FCC requirements and ITU recommendations for radio astronomy
              protection.

       1.6    Negotiation and signatures of this agreement are to be executed by PAC and the
              Electromagnetic Spectrum Management Unit of the National Science Foundation
              (NSF) for the Radio Astronomy sites identified in Section 2.1.

2.     National Science Foundation Radio Astronomy Observatories

       2.1    Radio Astronomy Site Listing

The Radio Astronomy sites under NSF support and listed in Table 2-1 make measurements in the
14.47-14.50 GHz band. These sites, including sites associated with the Very Long Baseline
Array (VLBA), are to be protected during their opera ion in accordance with the description
provided in Section 3.



                                              -2-


                         Table 2-1 Current Radio Astronomy Sites
                                                           Latitude                                    Longitude
                     Observatory
                                                           (D,M,S)                                      (D,M,S)
National Astronomy and Ionosphere Center (NAIC) site:

Arecibo, PR ........................................................................ 18 20 39      66 45 10

National Radio Astronomy Observatory OIRAO sites:

Green Bank Telescope, WV .............................................. 38 25 59                   79 50 23
Very Large Array, Socorro, NM ........................................ 34 04 44                    107 37 06

VLBA Sites:

St. Croix, VI .......................................................................   17 45 24   64 35 01
Hancock, NH ......................................................................      42 56 01   71 59 11
N. Liberty, IA......................................................................    41 46 17   91 34 27
Ft. Davis, TX ......................................................................    30 38 06   103 56 41
Los Alamos, NM ................................................................         35 46 30   106 14 44
Pie Town, NM ....................................................................       34 18 04   108 07 09
Kitt Peak, AZ .....................................................................     31 57 23   111 36 45
Owens Valley, CA .............................................................          37 13 54   118 16 37
Brewster, WA ....................................................................       48 07 52   119 41 00
Mauna Kea, HI ...................................................................       19 48 05   155 27 20

          2.2        Additional Radio Astronomy Sites

NSF may add new radio astronomy sites to the list given in Table 2-1. In this case NSF shall give
PAC at least 2 months notice of modifications to existing sites, o the inclusion of any additional
Radio Astronomy sites to operate in the 14.47 -14 5 GHz band.

3.        Operational Coordination Agreement

          NSF and PAC agree to the following stipulations:

          3.1        To provide protection to the Radio Astronomy sites listed in Table their
                     operational period, the following aggregate power flux density the 14.47-14.50
                     GHz band shall be no greater than:


                     (a)        -221 dB (W/m2/Hz) for the Arecibo, Green Bank and Socorro sites

                     (b)        -189 dB (W/m2/Hz) for the ten VLBA sites

          3.2        Within a year following initiation of the licensed PAC AMSS service, authorized
                     NSF and PAC personnel shall periodically review the terms of this Coordination



                                                                    -3-


               Agreement. If required, modifications of this Coordination Agreement will be
               negotiated and instituted.

      3.3      Any changes in the points of contact given in Section 5 shall be identified and
               reported by the respective party in a reasonable period.

      PAC agrees to the following stipulations:

      3.4      PAC will respond promptly to any NSF request for protection as described above
               for interference occurring at any site listed in Table 2-1.

      NSF agrees to the following stipulations:

      3.5      Provide PAC points of contact given in Section 5 a current schedule of Radio
               Astronomy measurements to be conducted in the 14.47-14.5 GHz band for the
               sites identified in Table 2-1.

      3.6      Via the National Astronomy and Ionosphere Center (NAIC) and the National
               Radio Astronomy Observatory (NRAO) provide PAC points of contact given in
               Section 5 any data that is not in accordance with the provisions in this
               Coordination Agreement.

4.    Termination Conditions

      4.1      This Coordination Agreement shall be binding for PAC and NSF.

      4.2      Either party providing a written notice of six months may execute termination of
               this Coordination Agreement.

5.    Points of Contact

      5.1      Points of contact for this Coordination Agreement are:


     Name:      Dr. Andrew W. Clegg                    Name:          Paul Sarraffe
     Organization: National Science Foundation         Organization: Panasonic Avionics
     Title: Program Director, ESMU                     Title:         eXConnect System
                                                                      Engineering
     Address: 4201 Wilson Boulevard,                   Address:       262000 Enterprise Way
                Room 1030
     City State Zip: Arlington VA 22230                City State Zip: Lake Forest, CA 92630
     Phone:     (703) 292-4892                         Phone:         (949) 672-2589
     Fax:       (703) 292-9034                         Fax:           (949) 462-7101
     E-mail:    esm@nsf.gov                            E-mail: paul.sarraffe@panasonic.aero




                                               -4-


          52—      Points of contact for Radio Astronomyobservation schedules are:


Dr          "Dr. Harvey Lisat


            NRAO                                                   onic Avionics Corporation
            520 Edgemont Rd.                                  262000 Enterprise Way
            Charlottesville, VA                               Lake Forest, CA                          |
           229032475                                          92630                                    |
            454—206—0544                                      (949) 672—2589
                434—29—0278                                   (949)462—7101        &          3
E—mail:         hlissl@nrao«do       _____                   ‘paulsarraffe@panesonic.aero _

6.         ignatures
             This Agreement is being made in goodfaith byboth parties and is effective on the
             date on which the last —party signs it
Forthe National Science Foundation                  For Panasonic Avioniss Corporation
                                                    By                      es
          Dr. Andrew W. Clegg                       Name: Anita Karti
          ProgramDirector, Electromagnetic          "itle:    Senior Director, Strategic Parterships
          SpectrumManagement Unit                          and eXConnect Regulatory Affairs
Date: December 18, 2009                             Date: December 18, 2009



Document Created: 2013-03-28 11:55:32
Document Modified: 2013-03-28 11:55:32

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