Request for Additional Location

0214-EX-ML-2015 Text Documents

Southwest Research Institute

2015-10-02ELS_167771

                                                         Southwest Research Institute
                                                Application for Modification of License
                                                             File No. 0214-EX-ML-2015

                   REQUEST FOR ADDITIONAL TEST LOCATION

Pursuant to Section 5.3 (f), Section 5.51 and Section 5.53 of the Federal
Communications Commission (“FCC”) rules, 47 C.F.R. §§ 5.3 (f), 5.51, 5.53 (2014),
Southwest Research Institute (“SwRI”) respectfully requests a modification of its
experimental license issued under call sign WF2XCH, 0294-EX-RR-2015, to add a
second, nearby test location at its campus for purposes of validation and verification of
radionavigation satellite service (“RNSS”) equipment associated with the Cyclone
Global Navigation Satellite System (“CYGNSS”).

In support of SwRI’s request, which is in compliance with NTIA Manual Paragraph
8.3.28, the following is shown:

1)    Applicant’s Address, Background and FRN:

      Southwest Research Institute is headquartered at 6220 Culebra Road, San
      Antonio, TX 78238-5166. It is an independent, not-for-profit, applied engineering
      and development organization devoted to technology research, design and
      development. It conducts business with the industry and government entities (in
      the U.S. and other friendly nations) on a worldwide basis. Approximately 50% of
      the SwRI’s business is for the U.S. Government. Its FCC Registration Number
      (“FRN”) is 0004074217.

2)    Background and Need for License Modification:

      The CYGNSS is a NASA funded system which will collect information related to
      hurricanes using GPS signals as a mechanism to detect wind speed. The system
      will use eight micro-satellites to measure wind speeds over Earth's oceans,
      increasing the ability of scientists to understand and predict hurricanes. Each
      satellite will take information based on the signals received from four GPS
      satellites. See https://www.nasa.gov/cygnss Thus, GPS signals are a
      fundamental element of the CYGNSS.

      The testing of CYGNSS satellites in production requires 'live sky' GPS signals for
      complete validation and verification of satellite hardware. Those signals need to
      be provided indoors due to cleanliness requirements during spacecraft
      construction. Accordingly, SwRI seeks a modification of its license so that it may
      to conduct tests at its indoor facilities identified below to obtain real-world data
      samples of the characteristics of CYGNSS transmissions. It acknowledges that
      such operation is limited to testing radionavigation satellite service equipment
      and systems.




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3)   Location of Additional Site:

     The proposed tests will be conducted on the campus of Southwest Research
     Institute, 6220 Culebra Road, San Antonio (Bexar County), Texas. The campus
     is comprised of approximately 1200 acres, and the location of the transmitter
     would be near the center of the campus. Thus, the nearest off-campus property
     is over 800 meters away.

     Specifically, the proposed tests will be conducted within Building 178, a site
     nearby where SwRI is already authorized to conduct related indoor GPS
     operations under its existing license, issued under call sign WF2XCH. The
     coordinates of the new site are NL 29-26-43; WL 98-37-31 (NAD 83).

4)   FCC Station Codes:

     The FCC radio service code and station class code for the proposed operation
     are “XT” and “FX,” respectively.

5)   Equipment To Be Used:

     SwRI proposes to operate a single transmitter capable of operating on the
     channels listed in Section 6. Specifically, it proposes to deploy a transmitter
     (Model L1/L2GHNRRKIT) manufactured by GPS Networking. The technical
     specifications of the equipment are provided under Attachment A.

6)   Frequencies Desired:

     As stated in Section 2 above, SwRI seeks to obtain real-world data samples of
     the characteristics of CYGNSS transmissions. Thus, it is critical for SwRI to
     conduct tests centered on GPS channels 1227.6 MHz and 1575.42 MHz. SwRI
     recognizes that the use of certain frequencies will require coordination through
     the Interdepartment Radio Advisory Committee (“IRAC”), and it is amendable to
     coordinating with Federal government personnel prior to commencing any
     transmissions.

7)   Power Level:

     SwRI will operate with the minimum necessary power to conduct its tests, and in
     no event will that level exceed the levels set out in the table provided under
     Attachment B. Specifically, the maximum equivalent isotropically radiated power
     (“EIRP”) will be such that the calculated emissions are no greater than -140
     dBm/24 MHz as received by an isotropic antenna at a distance of 100 feet (30
     meters) from the building where the tests are being conducted. A link budget
     showing compliance with this requirement is provided in the table under
     Attachment B and is based on free space propagation with no allowance for
     additional attenuation (e.g., building attenuation).




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8)    Type of Emission, Modulation Technique, and Bandwidth Required:

      The primary emission designator for the proposed operations is 2M46G3D, as
      indicated on the accompanying FCC Form. Other emission modes and
      modulation techniques may be utilized, but in no event will the emissions extend
      beyond the limits associated with the above-referenced emission.

      SWRI does not propose to supply station identification as set forth in Section
      5.115 of the Commission's Rules, 47 C.F.R. § 5.115 (2014),

9)    Antenna Information and Compliance with Human Exposure Limits:

      SwRI will comply with all Federal Aviation Administration (“FAA”) and FCC rules
      and regulations regarding the installation and operation of antennas and their
      support structures. The antenna to be deployed under the authority requested
      will not extend more than six meters more than six meters above the building.

10)   Restrictions on Operation:

      GPS users in the area of potential interference to GPS reception will be notified
      that GPS information may be impacted during testing. In addition, it will post
      signs on doors to the test area notifying that, "GPS re-radiator is in use and the
      GPS information you receive may be in error."

      SwRI also understands that: (a) permission to operate has been granted under
      experimental authority issued by the Federal Communications Commission, is
      strictly temporary, and may be cancelled at any time and that (b) operation is
      subject to the condition that it not cause harmful interference.

      Moreover, SwRI does not propose to market, sell, or lease unapproved
      equipment to end users or conduct a market study in conjunction with these
      tests. After the completion of the tests, SwRI will recover all devices that do not
      comply with FCC regulations.

11)   Interference Protection/Stop Buzzer Contact Information:

      As noted above, GPS users in the area of potential interference to GPS
      reception will be notified that GPS information may be impacted during testing.
      It also understands that it may be required to discontinue its operations immediately,
      if any interference occurs. SwRI does not expect interference to occur, however, as
      its tests will be conducted only on a limited basis and only periodically during the
      term of its experimental license. Moreover, SwRI personnel will be monitoring the
      RF spectrum and will take steps to minimize any potential for interference.

      In that regard, SwRI advises the Commission that Scott Thompson is the
      technical contact overseeing these tests. He will be personally responsible for
      the operations and will serve as the “stop buzzer” in the event that operations
      must be terminated because of any interference concerns. Mr. Thompson can
      be reached at (210) 522-6408, email sthompson@swri.org



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12)   Application Contact Information:

       Company Contact:                      “Stop Buzzer” Contact:

       Monica R. Trollinger                  Scott Thompson
       Deputy General Counsel                Space Science & Engineering, Div. 15
       6220 Culebra Road                        Space Science Directorate
       San Antonio, TX 78238-5166               Building 178, Office 206
       Telephone: (210) 522-6024             PO Drawer 28510
       Facsimile: (210) 522-5839             6220 Culebra Road
       mtrollinger@swri.org                  San Antonio, TX 78228-0510
                                             Telephone: (210) 522-6408
                                             sthompson@swri.org



       Legal Contacts:

       David E. Hilliard
       Kurt E. DeSoto
       Wiley Rein LLP
       1776 K Street, N.W.
       Washington, DC 20006
       Telephone: (202) 719-7000
       Facsimile: (202) 719-7207
       Email: dhilliard@wileyrein.com
       Email: kdesoto@wileyrein.com




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    ATTACHMENT A

Equipment Specifications




           5


                           L1/L2GHNRRKIT
                                        Technical Product Data
Features
   Amplified High Gain Roof Antenna (L1/L2/L5 Galileo/GLONASS and Omnistar)
      Gain  40dB

   Re-Radiating Amplifier with Power Supply
       Gain  20dB

   Optional Mounting Kit Hardware
        L1/L2GRAMB Roof Antenna Mount & WRUMT Re-Radiating Amp Mount

   Variable Gain Option Available
        Re-Radiating Amp Gain Varies from 0 to +20 dB


Description

The GPS L1/L2/L5 Galileo/GLONASS/Omnistar Hanger Networked Re-Radiating Kit
(L1/L2GHNRRKIT) is a complete re-radiating system that allows re-radiation of the GPS L1, L2, L5,
Galileo, GLONASS and Omnistar signals indoors. The L1/L2GHNRRKIT consists of an active roof
antenna, a re-radiating amplifier with a wall mount plug-in transformer that powers the entire system,
and a passive re-radiating antenna. The signal from the roof antenna is amplified and radiated
indoors. Thus, if a receiver has line of sight with the re-radiating antenna, it can receive all of the GNSS
signals indoors up to 100 feet away.

Re-Radiating Amplifier
                                               0
Electrical Specifications, TA = 25 C
Parameter              Conditions                                            Min     Typ     Max      Units
Freq. Range            Ant – J1                                              1.0             2.0      GHz
In/Out Imped.          Ant, J1                                                       50               
     (1)               Ant – J1, Normal Configuration
Gain                                                                         20      24.5    33       dB
                       Variable Gain Option                                  0               +20      dB
Input SWR             J1 - 50                                                               1.8:1    -
Output SWR            Ant - 50                                                              1.8:1    -
Noise Figure           Ant – J1                                                      2.4     2.7      dB
Gain Flatness         | L1 – L2 | ; Ant – J1                                         0.5     1        dB
Reverse Isolation      J1 – Ant                                              35                       dB
Group delay           d,max - d,min : Ant – J1                                             1        ns
Flatness
 (1) For performance plots, see LA20RPDC Data Sheet



REV. A                                              12/05/08                                              1


L1/L2/L5 Galileo/GLONASS Active Roof Antenna Specifications

Parameter          Conditions                           Min     Typ       Max       Units
Frequency          L1                                           1.575               GHz
                   L2                                           1.227               GHz
                   L5                                           1.176               GHz
                   Galileo L1                                   1.575               GHz
                   Galileo L2                                   1.278               GHz
                   GLONASS L1                                   1.602               GHz
                   GLONASS L2                                   1.246               GHz
                   Omnistar                                     1.535               GHz
Bandwidth                                                                           MHz
Out Imped.                                                      50                  
Pre-Amp Gain                                                    40                  dB
Noise Figure                                                    2.75                dB
Output SWR                                                                2.0:1     -
Req. DC Input V.                                        3.3               24        Vdc
Current                                                 20      35        40        mA


Re-Radiating Antenna

Electrical Specifications, TA = 250C
Parameter          Conditions                         Min     Typ                 Max         Units
Frequency          L1/L2/L5                                   1.575/1.227/1.176               GHz
                   Galileo                                    1.575/1.278                     GHz
                   GLONASS                                    1.602/1.246                     GHz
                   Omnistar                                   1.535                           GHz
Bandwidth                                                                         20          MHz
Impedance                                                     50                              
Peak Gain                                                     +3                  +3.5        dBic
VSWR                                                                              1.5:1
Polarization                                                  RHCP
DC Grounding       Lightning Protection                       YES



Mechanical Specifications (Passive L1/L2G Antenna)

Size: Diameter 2.60 in. (66.04 mm) Height: .64 in (16.18mm)
Weight: 4.06 oz. (115 Kg)
Finish: Skydrol Resistant Polyurethane Enamel, Base Iridite per MIL-C-5441
Color: Gloss White #17925 per FED STD-595B
Material: 6061-T6 ALUMINUM ALLOY BASE, THERMOSET PLASTIC
RADOME, UV, ABRASION & SKYDROL RESISTANCE
Connector: N-TYPE FEMALE



REV. A                                    12/05/08                                        2


Environmental Specifications (L1/L2/L5 Galileo/GLONASS Active/Passive Antennas)

Temperature: -67F to +185F (-55C to +85C)

Altitude: 70,000 Feet

Vibration: > 30G’s

Leakage: Hermetically Sealed

Federal and Military Specifications

Design to: FAA TSO-C144, DO-160D, MIL-C-5541, MIL-E-5400, MIL-I-45208A & MIL-STD-
810 and SAE J1455

Available Options

Re-Radiating Amp System Power Supply Options
  Source Voltage Options            VOLTAGE INPUT                           STYLE
                              110VAC                              Transformer (Wall Mount)
                              220 VAC                             Transformer (Wall Mount)
                              240 VAC (United Kingdom)            Transformer (Wall Mount)
                              Customer Supplied DC 9-32 VDC       Military Style Connector
Re-Radiating Amp Gain Control Options
  Normal Gain                 Gain  20 dB
  Variable Gain               0dB to +20dB
Re-Radiating Amp RF Connector Options
  Connector Options                 CONNECTOR STYLE                        CHARGE
                              Type N                              NC
                              Type SMA                            NC
                              Type TNC                            NC
                              Type BNC                            NC


Part Number

                                               VG L1/L2GHNRRKIT - N / 5 / 110

Gain Option:
       VG =Variable; Blank = Normal

Re-Radiator Frequencies
       L1/L2/L5 Galileo/GLONASS/Omnistar

Connector Options:
       N = N type; S = SMA; T = TNC; B = BNC

Output Voltage:
        5 = 5 VDC voltage to active antenna

Source Voltage
        110 -Transformer, 220 – Transformer, 240 – U.K. Transformer MC – Military Conn. (User
        supplies DC Voltage)




REV. A                                        12/05/08                                       3


                                            ATTACHMENT B

                                       Budget Link Calculations


The following calculations represent the architecture of SwRI’s proposed GPS re-radiation configuration
and the signal power calculations which demonstrates compliance with NTIA Manual 8.3.28.

                                                              Individual
                                                              element      Cumulative total

GPS signal received power from GPS spacecraft                    -130                -130 dBm

Receive Antenna pattern gain
(estimated)                                                        3                   -127

Receive Antenna amplifier gain
(data sheet)                                                      40                    -87

Transmission line loss to re-radiator antenna
(estimated)                                                       -27                  -114

Powered coaxial signal distribution splitter gain
(data sheet)                                                      14                   -100

Re-radiator amplifier
(data sheet)                                                      20                    -80

Re-radiator antenna gain
(estimated)                                                        3                    -77

Free space path loss (FSPL) at 100 feet inside Building 178       -66                -143 dBm


These calculations indicate that SwRI will not re-radiate GPS signals above -140dBm/24 MHz at 100 feet
from the re-radiation source.




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Document Created: 2015-10-01 11:34:46
Document Modified: 2015-10-01 11:34:46

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