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    sitelog navigation structure General Site Log Meteorological Data LAGEOS Performance Satellite Data Info

Herstmonceux: Site Log

Instructions and Update Site Log

You can use the hyperlinks to quickly get to the section of interest or you can scroll down to read them all.

Section: 0. Form
Section: 1. Identification of the Ranging System Reference Point (SRP)
Section: 2. Site Location Information
Section: 3. General System Information
Section: 4. Telescope Information
Section: 5. Laser System Information
Section: 6. Receiver System
Section: 7. Tracking Capabilities
Section: 8. Calibration
Section: 9. Time and Frequency Standards
Section: 10. Preprocessing Information
Section: 11. Aircraft Detection
Section: 12. Meteorological Instrumentation
Section: 13. Local Ties, Eccentricities, and Collocation Information
Section: 14. Local Events Possibly Affecting Computed Position
Section: 15. On-Site, Point of Contact Agency Information
Section: 16. Responsible Agency (if different from 15.)
Section: 17. More Information

       ILRS Site and System Information Form
       International Laser Ranging Service
 
  0.   Form
 
       Prepared by (Full Name)    : Philip Gibbs
       Preparer E-mail            : pgib@nerc.ac.uk
       Date Prepared              : 2004-10-04
       Report Type                : UPDATE
       Format Version             : 1.0
 
 
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  1.   Identification of the Ranging System Reference Point (SRP)
 
       Site Name                  : Herstmonceux
       IERS DOMES Number          : 13212S001
       CDP Pad ID                 : 7840
       Subnetwork                 : EUROLAS
       Description                : AZ EL INTERSECT
       Monument Description       : N.A.
       Monument Inscription       : N.A.
       Mark Description           : N.A.
       Date Installed             : 1982-01-01
       Date Removed               : (yyyy-mm-dd)
       Geologic Characteristic    : CLAYS/SANDSTONES
       Additional Information     : Local geology: The site is bounded to the
                                    south by old, but now drained, marshland
                                    with the English Channel about 6 km away.
                                    The underlying structure is interbedded
                                    clays and sandstones called the Hastings
                                    Beds. There is no history of seismic
                                    activity in the area.
 
 
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  2.   Site Location Information
 
       City or Town               : Hailsham
       State or Province          : East Sussex
       Country                    : UK
       Tectonic Plate             : Eurasian
       Approximate Position
         X coordinate          [m]: 4033463.1
         Y coordinate          [m]:   23662.8
         Z coordinate          [m]: 4924305.6
         Latitude            [deg]:      50.8674 N
         Longitude           [deg]:       0.3361 E
         Elevation             [m]:      75
       Additional Information     : The site is located in the grounds of
                                    Herstmonceux Castle
 
 
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  3.   General System Information
 
  3.01 System Name                : Herstmonceux
       4-Character Code           : HERL
       CDP System Number          : 35
       CDP Occupation Number      : 01
       Eccentricity to SRP (if Not Identical With SRP)
         North                 [m]: 0
         East                  [m]: 0
         Up                    [m]: 0
         Date Measured            : N.A.
       Date Installed             : 1982-01-01
       Date Removed               : (yyyy-mm-dd)
       Additional Information     : (multiple lines)
 
 
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  4.   Telescope Information
 
  4.01 Receiving Telescope Type   : CASSEGRAIN
         Aperture              [m]: 0.5
         Mount                    : AZ-EL
       Xmitting Telescope Type    : REFRACTOR
         Aperture              [m]: 0.1
       Tracking Camera Type       : TV thro main tel / TV on Celestron
         Model                    :
         Manufacturer             :
         Field of View       [deg]: 0.06 / 0.6
         Minimum Magnitude   [mag]: ~10  / ~8
       Transmit/Receive Path      : SEPARATE
       Transmit/Receive Switch    : NONE
       Max Slew Rate Az    [deg/s]: 20
       Max Slew Rate El    [deg/s]:  5
       Max Used Tracking Rate Az  : 20
       Max Used Tracking Rate El  :  5
       Telescope Shelter          : EYE-LID DOME, see additional information
       Daylight Filter Type       : Oven controlled spectral filter
       Dayl. Filt. Bandwidth  [nm]: 0.15
       Adjustable Attenuation     : NO
       Transmit Efficiency        : 0.7
       Receive Efficiency         : 0.7
       Date Installed             : 1998-06-26
       Date Removed               : (yyyy-mm-dd)
       Additional Information     : The dome's hemisphere is divided into 4
                                    segments (like segments of an orange) the 
                                    bottom two of which are fixed to a circular
                                    rail and the top two open by sliding over the
                                    bottom two. The whole structure can be
                                    rotated manually, normally only necessary to
                                    protect the telescope/observer from the wind
                                    since this scheme means that all the sky
                                    above 30 degrees elevation is available with
                                    the dome in any position. In normal operation
                                    the lowest part of the opening are East and
                                    West to provide access to the ground targets.
 
 
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  5.   Laser System Information
 
  5.01 Laser Type                 : ND:YAG
       Number of Amplifiers       : 2
       Primary Wavelength     [nm]: 1064
       Primary Maximum Energy [mJ]: Not used for ranging
       Secondary Wavelength   [nm]: 532
       Secondary Max. Energy  [mJ]: ~20
       Xmit Energy Adjustable     : NO
       Pulse Width (FWHM)     [ps]: ~100
       Max. Repetition Rate   [Hz]: 13
       Fullw. Beam Divergence  ["]: 5-200
       Final Beam Diameter     [m]: 0.03
       Eyesafe                    : NO
       Eyesafe Standard           : British Standard 4803
       Date Installed             : 1982-01-01
       Date Removed               : (yyyy-mm-dd)
       Additional Information     : An observer is always present at the 
                                    telescope during ranging and using a slaved
                                    radar system to detect aircraft close to
                                    the beam and kill the laser. For terrestrial
                                    calibration we insert a very large ND filter
                                    to render the beam eyesafe.
 
 
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  6.   Receiver System
 
  6.01.01 Primary Chain
          Wavelength          [nm]: 532
          Detector Type           : CSPAD
            Manufacturer          : PESO Consulting
            Model                 : 
            Quantum Efficiency [%]: ~20
            Nominal Gain          :
            Rise Time         [ps]: 1500
            Jitter (Single PE)[ps]: 30
            Field of View      ["]: 100 microns - see additional information
            Date Installed        : 1999-07-30
            Date Removed          : 2001-01-03
          Signal Processing       : N.A.
            Manufacturer          :
            Model                 :
            Date Installed        : (yyyy-mm-dd)
            Date Removed          : (yyyy-mm-dd)
            Amplitude Measurement : NO
            Return-rate Controlled: YES
            Mode of Operation     : Single Photon
          Time of Flight Observ.  : INTERVAL
            Manufacturer          : Stanford
            Model                 : 620
            Resolution        [ps]: 4
            Precision         [ps]: 30
            Date Installed        : 1995-01-01
            Date Removed          : (yyyy-mm-dd)
          Additional Information  : We have 4 Stanford counters of varying
                                    ages - for details of usage see SCH and
                                    SCI files. Our telescope has a field of 
                                    view of 10 arc minutes. However this is 
                                    reduced to a maximum of 250 arcsecs 
                                    because of an iris in the light path.
                                    For normal daytime observing we reduce
                                    the iris size to 50 arcsecs. For normal 
                                    night observing we use a 100 arcsecs iris.
                                    Whichever iris we use, the light is
                                    focused onto the detector.
 
  6.01.02 Primary Chain
          Wavelength          [nm]: 532
          Detector Type           : SPAD3b
            Manufacturer          : PESO Consulting
            Model                 : 
            Quantum Efficiency [%]: ~20
            Nominal Gain          :
            Rise Time         [ps]: 1500
            Jitter (Single PE)[ps]: 30
            Field of View      ["]: 100 microns - see additional information
            Date Installed        : 2001-01-03
            Date Removed          : 2001-01-24
          Signal Processing       : N.A.
            Manufacturer          :
            Model                 :
            Date Installed        : (yyyy-mm-dd)
            Date Removed          : (yyyy-mm-dd)
            Amplitude Measurement : NO
            Return-rate Controlled: YES
            Mode of Operation     : Single Photon
          Time of Flight Observ.  : INTERVAL
            Manufacturer          : Stanford
            Model                 : 620
            Resolution        [ps]: 4
            Precision         [ps]: 30
            Date Installed        : 1995-01-01
            Date Removed          : (yyyy-mm-dd)
          Additional Information  : We have 4 Stanford counters of varying
                                    ages - for details of usage see SCH and
                                    SCI files. Our telescope has a field of 
                                    view of 10 arc minutes. However this is 
                                    reduced to a maximum of 250 arcsecs 
                                    because of an iris in the light path.
                                    For normal daytime observing we reduce
                                    the iris size to 50 arcsecs. For normal 
                                    night observing we use a 100 arcsecs iris.
                                    Whichever iris we use, the light is
                                    focused onto the SPAD diode.
 
  6.01.03 Primary Chain
          Wavelength          [nm]: 532
          Detector Type           : CSPAD
            Manufacturer          : PESO Consulting
            Model                 : 
            Quantum Efficiency [%]: ~20
            Nominal Gain          :
            Rise Time         [ps]: 1500
            Jitter (Single PE)[ps]: 30
            Field of View      ["]: 100 microns - see additional information
            Date Installed        : 2001-01-24
            Date Removed          : 2002-10-04
          Signal Processing       : N.A.
            Manufacturer          :
            Model                 :
            Date Installed        : (yyyy-mm-dd)
            Date Removed          : (yyyy-mm-dd)
            Amplitude Measurement : NO
            Return-rate Controlled: YES
            Mode of Operation     : Single Photon
          Time of Flight Observ.  : INTERVAL
            Manufacturer          : Stanford
            Model                 : 620
            Resolution        [ps]: 4
            Precision         [ps]: 30
            Date Installed        : 1995-01-01
            Date Removed          : (yyyy-mm-dd)
          Additional Information  : We have 4 Stanford counters of varying
                                    ages - for details of usage see SCH and
                                    SCI files. Our telescope has a field of 
                                    view of 10 arc minutes. However this is 
                                    reduced to a maximum of 250 arcsecs 
                                    because of an iris in the light path.
                                    For normal daytime observing we reduce
                                    the iris size to 50 arcsecs. For normal 
                                    night observing we use a 100 arcsecs iris.
                                    Whichever iris we use, the light is
                                    focused onto the detector.
 
  6.01.04 Primary Chain
          Wavelength          [nm]: 532
          Detector Type           : SPAD3b
            Manufacturer          : PESO Consulting
            Model                 : 
            Quantum Efficiency [%]: ~20
            Nominal Gain          :
            Rise Time         [ps]: 1500
            Jitter (Single PE)[ps]: 30
            Field of View      ["]: 100 microns - see additional information
            Date Installed        : 2002-10-04
            Date Removed          : 2002-10-16
          Signal Processing       : N.A.
            Manufacturer          :
            Model                 :
            Date Installed        : (yyyy-mm-dd)
            Date Removed          : (yyyy-mm-dd)
            Amplitude Measurement : NO
            Return-rate Controlled: YES
            Mode of Operation     : Single Photon
          Time of Flight Observ.  : INTERVAL
            Manufacturer          : Stanford
            Model                 : 620
            Resolution        [ps]: 4
            Precision         [ps]: 30
            Date Installed        : 1995-01-01
            Date Removed          : (yyyy-mm-dd)
          Additional Information  : We have 4 Stanford counters of varying
                                    ages - for details of usage see SCH and
                                    SCI files. Our telescope has a field of 
                                    view of 10 arc minutes. However this is 
                                    reduced to a maximum of 250 arcsecs 
                                    because of an iris in the light path.
                                    For normal daytime observing we reduce
                                    the iris size to 50 arcsecs. For normal 
                                    night observing we use a 100 arcsecs iris.
                                    Whichever iris we use, the light is
                                    focused onto the SPAD diode.
 
  6.01.05 Primary Chain
          Wavelength          [nm]: 532
          Detector Type           : CSPAD
            Manufacturer          : PESO Consulting
            Model                 : 
            Quantum Efficiency [%]: ~20
            Nominal Gain          :
            Rise Time         [ps]: 1500
            Jitter (Single PE)[ps]: 30
            Field of View      ["]: 100 microns - see additional information
            Date Installed        : 2002-10-16
            Date Removed          : (yyyy-mm-dd)
          Signal Processing       : N.A.
            Manufacturer          :
            Model                 :
            Date Installed        : (yyyy-mm-dd)
            Date Removed          : (yyyy-mm-dd)
            Amplitude Measurement : NO
            Return-rate Controlled: YES
            Mode of Operation     : Single Photon
          Time of Flight Observ.  : INTERVAL
            Manufacturer          : Stanford
            Model                 : 620
            Resolution        [ps]: 4
            Precision         [ps]: 30
            Date Installed        : 1995-01-01
            Date Removed          : (yyyy-mm-dd)
          Additional Information  : We have 4 Stanford counters of varying
                                    ages - for details of usage see SCH and
                                    SCI files. Our telescope has a field of 
                                    view of 10 arc minutes. However this is 
                                    reduced to a maximum of 250 arcsecs 
                                    because of an iris in the light path.
                                    For normal daytime observing we reduce
                                    the iris size to 50 arcsecs. For normal 
                                    night observing we use a 100 arcsecs iris.
                                    Whichever iris we use, the light is
                                    focused onto the detector.
 
 
  Back to top
 
 
  7.   Tracking Capabilities
 
  7.01 Satellites
         Very Low Alt (<400 km)   : YES
         Low Altitude (400-2000)  : YES
         Lageos                   : YES
         GLONASS                  : YES
         Etalon                   : YES
         GPS                      : NIGHT
         Moon                     : NO
       Avge Pass Switch Time   [s]: ~30
       Average values for Lageos
         Single Shot RMS      [mm]: 16
         # of Obs per NP          : 150
         Use of Semi-trains       : YES
         # of Semi-train Tracks   : 4
       Range Gate Width       [ns]: 200-30000 see additional info
       Beam Pointing Accuracy  ["]: 2
       Angle Encoder Resolution["]: 2
       Min. Tracking Elev.   [deg]: 30 in daylight  25 during nighttime
       Operation
         Months per Year          :  12
         Days per Week            :   7
         Hours per Day            : ~20
         Staff per Shift          :   1
         System Shared With       : NOTHING
         Time Allocated to SLR [%]: 100
         Remotely Controllable    : NO
       Date First Applicable      : 1982-01-01
       Date Last Applicable       : (yyyy-mm-dd)
       Additional Information     : If we use no ND then the daytime limit is of order
                                    600ns. However for low satellites we can put in
                                    considerable ND and use a range gate of 3000ns. In
                                    practice we will keep a small range gate <500ns for low
                                    satellites and using time bias corrections bring the
                                    satellite into the range gate.
                                    At night time we can have a RG of 30000ns
 
  Back to top
 
 
  8.   Calibration
 
  8.01 Calibration Type           : PRE+POST
       Target Location            : EXTERNAL
       Target Type                : see additional information
       Target Structure           : BRICK BUILDING, see additional information
       Target Distance         [m]: 120
         Date Measured            : 1993-06-09 -remeasured 2002
         Accuracy (mm)        [mm]: 2-3
         Verification             : 4 other targets
       Return-rate Controlled     : YES
       Mode of Operation          : SINGLE
       Average Cal Interval  [min]: 60 see additional information
       Single Shot RMS        [mm]: 9
       Edit Criterion 1st Chain   : ITERATIVE 2.5 SIGMA
       Edit Criterion 2nd Chain   : N.A.
       Application of Cal Data    : LINEAR FIT
       Date Installed             : 1982-01-01
       Date Removed               : (yyyy-mm-dd)
       Additional Information     : Targets are made of two polished steel
                                    sheets at right angles so as to
                                    translate the beam horizontally from
                                    the emitter telescope to the receiving
                                    telescope.  The 2 polished sheets are
                                    mounted on brick building about 30 feet
                                    above the ground, 120m from dome. A
                                    secondary target of 2 polished sheets is
                                    mounted on standard concrete survey
                                    pillar about 3 feet above the ground
                                    at 600m.
 
                                    We will always attempt to get calibrations 
                                    before and after satellite but when there 
                                    are several satellites back-to-back we will 
                                    calibrate before and after the batch. The 
                                    realtime system gives alarm messages should
                                    the time since last calibration exceed 60 
                                    minutes
 
  Back to top
 
 
  9.   Time and Frequency Standards
 
  9.01.01 Frequency Standard Type : Crystal Oscillator
          Model                   : 2110
          Manufacturer            : Austron
          Short Term Stab.  [e-12]: <3
          Long Term Stab.   [e-12]: 1
          Time Reference          : GPS
          Synchronization         : GPS
          Epoch Accuracy      [ns]: 100-300  
          Date Installed          : 1996-06-19
          Date Removed            : (yyyy-mm-dd)
          Additional Information  : Epoch accuracy not measured explicitly.
                                    A 10 MHz signal from the Datum GPS 
                                    receiver is feed to the Austron 
                                    Disciplined Frequency and that output
                                    is used for our time interval frequency.
 
  9.02.01 GPS Timing Rcvr Model   : 9390-52133
          Manufacturer            : Datum
          Date Installed          : 1995-01-01
          Date Removed            : (yyyy-mm-dd)
          Additional Information  : (multiple lines)
 
 
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 10.   Preprocessing Information
 
 10.01 On-site NP Generation      : YES
       Data Screening             : Orbit solution (SOLVE) + Gaussian fit
       Edit Criterion 1st Chain   : 3.0 SIGMA
       Edit Criterion 2nd Chain   : N.A.
       Upload interval            : ASAP - normally within 60mins
       Date First Applicable      : 1982-01-01
       Date Last Applicable       : (yyyy-mm-dd)
       Additional Information     : (multiple lines)
 
 
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 11.   Aircraft Detection
 
 11.01 Detection Type             : RADAR
       Date Installed             : 1984-01-01 Upgraded 2003
       Date Removed               : (yyyy-mm-dd)
       Additional Information     : Observer always on the observing
                                    platform during ranging to satellites
 
 
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 12.   Meteorological Instrumentation
 
 12.01.01 Pressure Sensor Model   : DPI 141
          Manufacturer            : Druck
          Recording Interval      : EVERY 5 MINUTES
          Accuracy          [mbar]: 0.15
          Height Diff to SRP   [m]: 0
          Date Installed          : 1999-06-29
          Calibration Interval    : see below
          Date Removed            : (yyyy-mm-dd hh:mm UT)
          Additional Information  : Pressures continuously compared with
                                    results from second Druck and with local
                                    mercury and Met Office barometers
 
 12.02.01 Temp Sensor Model       : HMP 140
          Manufacturer            : Vaisala
          Recording Interval      : EVERY 5 MINUTES
          Accuracy         [deg C]: 0.1
          Date Installed          : 1997-07-04
          Calibration Interval    : see below
          Date Removed            : 2001-12-18
          Additional Information  : Temperatures continuously compared with
                                    results from another temperature sensor
                                    and with local Met Office readings
 
 12.02.02 Temp Sensor Model       : MP103A-T7-W4W
          Manufacturer            : Rotronics
          Recording Interval      : EVERY 5 MINUTES
          Accuracy         [deg C]: 0.1
          Date Installed          : 2001-12-18
          Calibration Interval    : see below
          Date Removed            : (yyyy-mm-dd hh:mm UT)
          Additional Information  : Temperatures continuously compared with
                                    results from another temperature sensor
                                    and with local Met Office readings
 
 12.03.01 Humidity Sensor Model   : HMP 140
          Manufacturer            : Vaisala
          Recording Interval      : EVERY 5 MINUTES
          Accuracy       [% rel h]: 5
          Date Installed          : 1996-06-19
          Calibration Interval    : see below
          Date Removed            : 2001-12-18
          Additional Information  : Relative humidities continuously compared
                                    with results from another device and with
                                    local Met Office readings
 
 12.03.02 Humidity Sensor Model   : MP103A-T7-W4W
          Manufacturer            : Rotronics
          Recording Interval      : EVERY 5 MINUTES
          Accuracy       [% rel h]: 1.5
          Date Installed          : 2001-12-18
          Calibration Interval    : see below
          Date Removed            : 
          Additional Information  : Relative humidities continuously compared
                                    with results from another device and with
                                    local Met Office readings
 
  Back to top
 
 
 13.   Local Ties, Eccentricities, and Collocation Information
 
 13.01 Collocated Permanent Geodetic Systems
 
       GPS                        : IGS+EUREF
         Date Installed           : (yyyy-mm-dd)
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       GLONASS                    : IGS+EUREF+IGLOS
         Date Installed           : 2003-03-01
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       DORIS                      : NO
         Date Installed           : (yyyy-mm-dd)
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       PRARE                      : NO
         Date Installed           : (yyyy-mm-dd)
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       VLBI                       : NO
         Date Installed           : (yyyy-mm-dd)
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       Gravimeter                 : NO
         Date Installed           : (yyyy-mm-dd)
         Date Removed             : (yyyy-mm-dd)
         Additional Information   : (multiple lines)
       etc
 
 13.02.01 Local Ties from the SRP to Other Monuments or Systems on Site
 
          Monument Name           : HERS
          Instrumentation Type    : GPS
          Instrumentation Status  : PERMANENT
          DOMES Number            : 13212M007
          CDP Number              : (XXXX)
          Differential Components (ITRS)
            dx                 [m]:  +6.505 +- 0.002
            dy                 [m]: +10.278 +- 0.002
            dz                 [m]:  -3.945 +- 0.002
            Date Measured         : 1992-07-29
            Determined by         : UK Ordnance Survey
          Date Installed          : 1998-07-01
          Date Removed            : (yyyy-mm-dd)
          Additional Information  : IGS code for the GPS is HERS
 
 13.02.02 Local Ties from the SRP to Other Monuments or Systems on Site
 
          Monument Name           : HERT
          Instrumentation Type    : GPS+GLONASS
          Instrumentation Status  : PERMANENT
          DOMES Number            : 13212M010
          CDP Number              : (XXXX)
          Differential Components (ITRS)
            dx                 [m]:  -2.674 +- 0.002
            dy                 [m]: -124.815 +- 0.002
            dz                 [m]:  +12.995 +- 0.002
            Date Measured         : 2003-03-12
            Determined by         : GPS CAMPAIGN/TRIANGULATION
          Date Installed          : 2003-03-01
          Date Removed            : (yyyy-mm-dd)
          Additional Information  : IGS code for the GPS is HERT
 
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 14.   Local Events Possibly Affecting Computed Position
 
 14.01 Date                       : (yyyy-mm-dd hh:mm UT)
       Event                      : (EARTHQUAKE/CONSTRUCTION/etc)
       Additional Information     : (multiple lines)
 
 
  Back to top
 
 
 15.   On-Site, Point of Contact Agency Information
 
       Agency                     : Natural Environment Research Council
       Mailing Address            : NERC Space Geodesy Facility
                                    Herstmonceux Castle
                                    Hailsham
                                    East Sussex BN27 1RN
       Primary Contact
         Contact Name             : Dr Graham Appleby
         Telephone (primary)      : +44 (0)1323 833888
         Telephone (secondary)    : +44 (0)1487 772477
         Fax                      : +44 (0)1323 833929/+44 (0)1487773467
         E-mail                   : gapp@nerc.ac.uk 
       Secondary Contact
         Contact Name             : Philip Gibbs
         Telephone (primary)      : +44 (0)1323 833888
         Telephone (secondary)    :
         Fax                      : +44 (0)1323 833929
         E-mail                   : pgib@nerc.ac.uk 
       Additional Information     : (multiple lines)
 
 
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 16.   Responsible Agency (if different from 15.)
 
       Agency                     : (multiple lines)
       Mailing Address            : (multiple lines)
       Primary Contact
         Contact Name             :
         Telephone (primary)      :
         Telephone (secondary)    :
         Fax                      :
         E-mail                   :
       Secondary Contact
         Contact Name             :
         Telephone (primary)      :
         Telephone (secondary)    :
         Fax                      :
         E-mail                   :
       Additional Information     : (multiple lines)
 
 
  Back to top
 
 
 17.   More Information
 
       URL for More Information   : http://nercslr.nmt.ac.uk/
       Hardcopy on File
         Site Map                 : NO
         Site Diagram             : NO
         Horizon Mask             : NO
         Monument Description     : NO
         Site Pictures            : NO
       Additional Information     : (multiple lines)
 
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