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National Space Science Center
            Chinese Academy of Sciences




    PROGRESSES OF DEVELOPMENT OF
       CFOSAT SCATTEROMETER

                                       Xiaolong Dong, Di Zhu
                          CAS Key Laboratory of Microwave Remote Sensing
                                 National Space Science Center, CAS
                                    PO Box 8701, Beijing, China
                            dongxiaolong@mirslab.cn, zhudi@mirslab.cn


IGARSS 2012, Munich, Germany                               Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                           Chinese Academy of Sciences
                                                                                          (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                Outline of the Presentation

•        Introduction to the Mission
•        Specifications of SCAT
•        Description of SCAT system
•        Simulation of SCAT system
         performances
•        Progresses
•        Summary

IGARSS 2012, Munich, Germany                    Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                Chinese Academy of Sciences
                                                                               (MiRS, CAS)
National Space Science Center
                Chinese Academy of Sciences

                                                        •   Two payloads:
     CFOSAT Mission                                          – SWIM (Sea Wave Investigation and
                                                               Monitoring by satellite)
                                                                 • A Ku-band real aperture radar for
•     CFOSAT: Chinese French Oceanography                          measurement of directional ocean
                                                                   wave spectra;
      SATellie
                                                             – SCAT (SCATterometer)
•     Launch plan: 2014
                                                                 • A Ku-band rotating fan-beam radar
•     Mission Objectives:                                          scatterometer for measurement of
     monitoring the wind and waves at the ocean                    ocean surface wind vector.
     surface at the global scale in order to improve:
      – The wind and wave forecast for marine
          meteorology (including severe events)
      – the ocean dynamics modeling and
          prediction,
      – our knowledge of climate variability
      – fundamental knowledge on surface
          processes linked to wind and waves



    IGARSS 2012, Munich, Germany                                   Key Laboratory of Microwave Remote Sensing
    July 22-27, 2012                                                               Chinese Academy of Sciences
                                                                                                  (MiRS, CAS)
National Space Science Center
              Chinese Academy of Sciences




         Mission-measurement requirements
• Joint measurement of ocean surface wind vector
  and sea-state parameters from radar
   – Both wind vector and wave parameters can be measured using active micro-wave
     remote sensing (heritage of altimeter, sactterometer and SAR missions, and airborne
     radar measurements)
   – Wind vector => optimal configuration at medium incidence angle (20-50°)
   – Wave spectra => optimal configuration at low incidence angle (< 15°)


• CFOSAT mission with two payloads
   – SWIM: wave scatterometer: multi-beam Ku-Band radar at low incidence
   – SCAT: wind scatteromer: Fan beam Ku-Band radar at medium incidence


  IGARSS 2012, Munich, Germany                           Key Laboratory of Microwave Remote Sensing
  4
  July 22-27, 2012                                                       Chinese Academy of Sciences
                                                                                        (MiRS, CAS)    4
National Space Science Center
            Chinese Academy of Sciences



            Mission-Wind Vector Payload -SCAT
•   A Ku-band rotating fan-beam radar
    scatterometer (Ku-RFSCAT) for sea
    surface wind vector retrieval by
    measurement of the sea surface
    backscattering coefficient.                                   Rotating fan-beam antenna
•   Adapted to the platform constraints
    (small size);
•   2 fan beams (HH & VV) cover incident        Nadir Point
    angles from 26 degree to 46 degree
    from nadir
•   scanned with a rotation speed of around           footprint
    3.5 rpm.
•   For each of the ground resolution cells,
    more than four looking angles can be
    obtained to retrieval wind vector
    information.



IGARSS 2012, Munich, Germany                       Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                            5                      Chinese Academy of Sciences
                                                                                  (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                         Characteristics of CFOSAT SCAT
• Wide swath by rotating of beam;
      – Decided by outer edge of incident angle of beam
• More number of azimuth look angles by overlap of beam;
      – Decided by flying speed, rotating speed and beamwidth
• NRCS/sigma 0 dependent on antenna beam;
      – Decided by local antenna gain along elevation
• Single antenna for all azimuth directions;
      – No inter-beam balance required
      – But azimuth fluctuation may exist due to rotating mechanism




IGARSS 2012, Munich, Germany                    Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                Chinese Academy of Sciences
                                                                               (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                               Azimuth look angle combinations
                                  for surface resolution cells
           Overlap between adjacent scanns
           for large number of azimuth view for
           each pixel. Dual polarization is used                 Surface resolution cell 1
           to improve retrieval of outer and
           center part of the swath



                                                                                         Track of nadir porints




                                            Surface resolution cell 2


IGARSS 2012, Munich, Germany                                                       Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                                   Chinese Academy of Sciences
                                                                                                                  (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Specifications for SCAT
• Objectives:
      – Measurement of global surface sigma 0
      – Retrieval of global ocean surface wind vector
• Data requirements
      – Swath width: >1000km
      – Surface resolution: 50km (standard); 25km (goal)
      – Data quality (at 50km resolution)
      – ° precision:
              • 1.0dB for wind speed 4~6m/s
              • 0.5dB for wind speed 6~24m/s
      – Wind speed: 2m/s or 10% @ 4~25m/s
      – Wind direction: 20deg @ 360deg for most part of the swath
• Life time: 3yrs

IGARSS 2012, Munich, Germany                              Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                          Chinese Academy of Sciences
                                                                                         (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Specifications of SCAT

                             Ku-RFSCAT                           Parameters
Antenna Spinning rate :                                 3.5 rpm
Polarization:                                           VV, HH
PRF/channel:                                            75 Hz/channel
Pulse peak power (Pt):                                  120 W
Pulse bandwidth (B):                                    0.5 MHz
Pulse duration (τp):                                    1.3 ms
Swath width:                                            1000 km
Receive gate length(Tg):                                2.82 ms
Receive gate delay:                                     3.74 ms
Inclination:                                            97.5 deg

IGARSS 2012, Munich, Germany                              Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                          Chinese Academy of Sciences
                                                                                         (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                Description of SCAT system
•    System overview
•    Choice of system type
•    Operation mode
•    System configuration
•    Key parameters




IGARSS 2012, Munich, Germany                   Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                               Chinese Academy of Sciences
                                                                              (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            System overview
• Ku-band rotating fan-beam scatterometer
      – Platform dimension
      – Technology heritage
      – Available GMFs
• Long LMF pulse with de-ramp pulse compression
      – TX: 1.35ms
      – RX: 2.72 ms
• Digital I-Q receiver with on-board pulse compression
  processing and resolution cell regrouping
• TX/RX channel except antenna and switch matrix
  identical primary/backup design to ensure liability

IGARSS 2012, Munich, Germany                          Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                      Chinese Academy of Sciences
                                                                                     (MiRS, CAS)
National Space Science Center
             Chinese Academy of Sciences

                                             Choice of system type
                                             -Why rotating fan beam?

• Why rotating beam?                                 • Why rotating fan beam?
    – Overlap of surface coverage with                  – Lower rotating speed to ensure
      SWIM is requirement, nadir gap                      life time of rotating mechanism;
      should be avoided.                                – Multiple incident angles for
    – Deployment of multiple fan-beam                     better wind direction retrieval;
      antenna is not allowed due to                     – Large incident angle ranges
      platform capability.                                (20~46°) for investigation of
    – Large swath at a relatively low                     ocean surface scattering
      orbit (~500km) requires scanning.                   characteristics, by compensating
                                                          with SWIM (0~10°)



 IGARSS 2012, Munich, Germany                                 Key Laboratory of Microwave Remote Sensing
 July 22-27, 2012                                                             Chinese Academy of Sciences
                                                                                             (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Other constraints
•    Antenna dimension: <1.2m
•    Available Pulsed Ku-TWTA: <140W
•    Available TWTA PRF: >150Hz
•    Data rate: <220kpbs
•    Rotating speed and mechanism lifetime




IGARSS 2012, Munich, Germany                           Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                       Chinese Academy of Sciences
                                                                                      (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Operation mode
• Normal mode: dual polarization with rotation;
• Test/cal mode:
      – raw waveform with lower PRF;
      – Including both rotating mode and fixed pointing
        mode;
• Single polarization mode



IGARSS 2012, Munich, Germany                         Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                     Chinese Academy of Sciences
                                                                                    (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            System configuration
•    Antenna subsystem                             •   Power amplifier subsystem
      – Antenna and feeding network;                    – TWT and EPC
      – Scanning mechanism;                        •   Digital subsystem
      – Servo controller;                               –   Signal generator;
•    RF subsystem                                       –   System controller;
      – Switch matrix;                                  –   Signal processor;
      – RF receiver;                                    –   Communication controller;
•    RX/TX electronics subsystem                   •   Secondary power supply subsystem
      – IF receiver;                                    – DC-DC power converter;
      – Frequency synthesizers;                         – TC/TM module
      – TX up-converter                            •   WG & cable assembly




IGARSS 2012, Munich, Germany                                    Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                Chinese Academy of Sciences
                                                                                               (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                                                                                          System Diagram
IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)
National Space Science Center
             Chinese Academy of Sciences



System configuration

 • Interface with structure
   subsystem
      – Antenna and part of the
        servo mechanism installed
        outside the satellite;
      – Other equipments
        installed inside the
        satelltie

 IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
 July 22-27, 2012                                            Chinese Academy of Sciences
                                                                            (MiRS, CAS)
Basic radar parameters
                          Parameter                    Specifications

                          Frequency                     13.256GHz

                      Signal bandwidth                    0.5MHz

               Internal calibration precision        Better than 0.15dB
                         Receiver NF                      ≤2.0dB
                Insertion loss of TX channel              ≤1.5dB

                Insertion loss of RX channel              ≤3.0dB

                 Transmitting power (peak)                 120W
                         Pulse width                      1.35ms
                              PRF                      2×75=150Hz



EUMETSAT/ESA Scatterometer Science Conference 2011
April 11-13, Darmstadt, Germany
National Space Science Center
            Chinese Academy of Sciences


                          Optimization of radar parameters

• Optimization:
   trade-off between SNR, measurement
  samples of each look and number of looks.
   maximization of wind vector retrieval
  performance
      – Surface resolution
      – Signal bandwidth
      – Rotating speed
IGARSS 2012, Munich, Germany                 Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                             Chinese Academy of Sciences
                                                                            (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences
                                    Resolution in azimuth direction
                                       & azimuth beam-width
• Fan beamlower gainantenna as long as
  possible
• Decided by antenna beamwidth
• Limited by satellite dimension: ≤1.2m
• Beamwidth ~1.1 deg resolution in azimuth
  direction: 10.5~14.5km



IGARSS 2012, Munich, Germany                           Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                       Chinese Academy of Sciences
                                                                                      (MiRS, CAS)
Design of rotating speed
     •    Trade-off between independent
          sigma 0measuremrent samples for
          single look and number of looks
     •    Optimization of 3.5rpm




EUMETSAT/ESA Scatterometer Science Conference 2011
April 11-13, Darmstadt, Germany
National Space Science Center
              Chinese Academy of Sciences
                                    Resolution in elevation direction
                                          & signal bandwidth

• Low SNR due to low antenna
   gain
• Bandwidth 0.5MHz
  resolution:380~650m
• On-board non-coherent re-
   grouping to improve sigma 0
   precision
  resolution of 5km



  IGARSS 2012, Munich, Germany                          Key Laboratory of Microwave Remote Sensing
  July 22-27, 2012                                                      Chinese Academy of Sciences
                                                                                       (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                                  Onboard processing
 • Reduce data rate to ~220kbps
 • Downlink data resolution: ~10km(az) × 5km(el)
        – (original resolution: 10km(az) × (<1km(el))
 • Signal+noise processing & noise-only processing




IGARSS 2012, Munich, Germany                            Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                        Chinese Academy of Sciences
                                                                                       (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                     Internal Calibration Loop
                                                                                     P1
                                K1
                                                        C1             LPF1
                                                                                            P31
                  P21                 Circulator                                          TWTA
                  P22                                                                       P32

                                                                                 K6




                                                   C2        K2
                            D                                     K3                      K5
                                             A
                            Ns                                                LPF2
                                                 K4                                               P31

                                                                                                  P32

                                                                  Compositions:
                                                                  •C1,C2:directional couplers
                              Ports:                              •K1,K2,K3,K4:ferrite switches
                              •P1: BJ-140 to TWTA                 •K5,K6:mechanical switches
                              •P2: BJ-140 to antennas             •LPF1/2:EMC filters
                              •P3: BJ-140 to RF receiver          •D: power monitoring detector
                                                                  •Ns:internal noise source

IGARSS 2012, Munich, Germany                                                          Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                                      Chinese Academy of Sciences
                                                                                                                     (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                            Simulations of system performances

• Simulation model
• Simulation of         precision
• Simulation of wind vector retrieval
  performance




IGARSS 2012, Munich, Germany                    Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                Chinese Academy of Sciences
                                                                               (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                                            Simulation model




IGARSS 2012, Munich, Germany                              Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                          Chinese Academy of Sciences
                                                                                         (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                  Simulation of ° precision
• Modeling                                                   2
                                                                     G2 
                                               Pr   Pt                    dA              SNR SNR 
      – Radar equation
                                                             3          4
                                 L                       4       A
                                                                      R                       Pr
                       where:                                                                 N
      – SNR            P 120W 50.8dBm           t                                              1                       2
                                                                                                                                   G2 
                                                                                                  Pt                                    dA
      – ° precision
                                                                                                                       3
                          2.263cm 16.5dB                                                      kBT    4                     L   A
                                                                                                                                    R4
                                               L 3.5dB (insturment loss)

                                                                        2                                          2
                                 
                 P              true         1         1                       1                      1
       Kp                      
                                                 1               
                                                                                        1                   
                 P             true         Neff   SNR           true       Nnoise            SNR           true


      Kp(dB) 10log 1 Kp

IGARSS 2012, Munich, Germany                                                       Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                                   Chinese Academy of Sciences
                                                                                                                  (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


• Statistics:
  number of looks (left)
  number of independent samples (right)




IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)
National Space Science Center
                     Chinese Academy of Sciences



  SNR distribution


                                                     U=4m/s            U=8m/s




IGARSS 2012, Munich, Germany                         U=16m/s          U=24m/s
                                                               Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                               Chinese Academy of Sciences
                                                                                              (MiRS, CAS)
National Space Science Center
                           Chinese Academy of Sciences



  Kp distribution (25km)


                                                           U=4m/s            U=8m/s




IGARSS 2012, Munich, Germany                               U=16m/s          U=24m/s
                                                                     Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                     Chinese Academy of Sciences
                                                                                                    (MiRS, CAS)
National Space Science Center
             Chinese Academy of Sciences


                                Simulation of wind retrieval

• Only °data with precision better than 1.0dB will be used for
  wind retrieval;
• Standard MLE method and NSCAT GMF are used for simulation;
• Median filter algorithm for wind direction ambiguity removal




• 2 kinds of wind field simulated
     – Spatially correlated parallel wind field and circular wind field
     – Random wind field

 IGARSS 2012, Munich, Germany                          Key Laboratory of Microwave Remote Sensing
 July 22-27, 2012                                                      Chinese Academy of Sciences
                                                                                      (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                                   Parallel and circular wind field
                                              (U~[2,24])




IGARSS 2012, Munich, Germany                            Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                        Chinese Academy of Sciences
                                                                                       (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences



                         Retrieval performance of parallel wind
                                          field

        U                       Qe(m/s)-U   QRMS(m/s)-U   Qe (o)-phi                 QRMS (o)-phi
         4                         0.43        0.65         51.5                        65.9
         6                         0.45        0.66         15.9                        22.3
         8                         0.55        0.76         10.9                        16.5
        10                         0.68        0.93         10.1                        15.4
        12                         0.83        1.13         10.2                        15.6
        14                         0.99        1.33         10.3                        15.7
        16                         1.17        1.57         10.8                        16.3
        18                         1.38        1.83         11.3                        17.0
        20                         1.60        2.12         12.1                        18.1
        22                         1.86        2.43         12.9                        19.1
        24                         2.13        2.75         13.4                        19.8



IGARSS 2012, Munich, Germany                              Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                          Chinese Academy of Sciences
                                                                                         (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences
                         Retrieval performance of circular wind
                                          field

       U                     Qe(m/s)-U      QRMS(m/s)-U   Qe (o)-phi              QRMS (o)-phi
        4                       0.44           0.68         39.1                     51.9
        6                       0.46           0.68         15.6                     22.3
        8                       0.55           0.77         10.9                     16.6
       10                       0.69           0.95         10.2                     15.7
       12                       0.86           1.17         10.4                     16.0
       14                       1.02           1.38         10.6                     16.3
       16                       1.22           1.62         11.1                     16.9
       18                       1.44           1.90         11.8                     17.8
       20                       1.68           2.20         12.7                     19.0
       22                       1.93           2.51         13.5                     20.0
       24                       2.19           2.83         14.0                     20.7




IGARSS 2012, Munich, Germany                                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                            Chinese Academy of Sciences
                                                                                           (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                      FOM varying with wind speed




IGARSS 2012, Munich, Germany                          Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                      Chinese Academy of Sciences
                                                                                     (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Random wind field
•    Parallel wind field simulated
•    Wind speed range: 4~24m/s
•    Wind direction search interval: 10deg
•    25km WVC resolution




IGARSS 2012, Munich, Germany                           Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                       Chinese Academy of Sciences
                                                                                      (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences



  U=4m/s
  U=8m/s




IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences



  U=16m/s
  U=12m/s




IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences



  U=24m/s
  U=20m/s




IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                        Wind vector retrieval performance

                                            RMS of wind speed   RMS of wind direction
   Input wind speed                              (m/s)                  (o)

                4                                  0.7                          35.5
                6                                  0.7                          22.3
                8                                  0.8                          16.6
               10                                  1.0                          15.7
               12                                  1.2                          16.0
               14                                  1.4                          16.3
               16                                  1.6                          16.9
               18                                  1.9                          17.8
               20                                  2.2                          19.0
               22                                  2.5                          20.0
               24                                  2.8                          20.7
IGARSS 2012, Munich, Germany                                    Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                Chinese Academy of Sciences
                                                                                               (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Retrieval performance

                              Near nadir             Far range within footprint Near range within footprint
                             (-100~+100)                     (>400km)                  (100~400km)
U(m/s)
                         0           U        phi         0       U        phi                 0             U         phi
                     (dB)           (m/s)     ( )       (dB)     (m/s)     ( )              (dB)            (m/s)      ( )

    4            0.89-1.79           0.4      44.1   1.43-3.07    1.1     44.7          0.66-2.07             0.4      31.8
    8            0.46-0.66           0.9      24.2   0.51-1.01    1.3     26.9          0.44-0.74             0.6      11.0
   12            0.41-0.53           1.2      22.7   0.45-0.63    1.8     26.6          0.41-0.54             0.9      10.4
   16            0.40-0.49           2.1      22.7   0.44-0.54    2.2     27.6          0.40-0.49             1.3      11.3
   20            0.40-0.48           2.9      24.8   0.43-0.50    2.9     30.1          0.40-0.47             1.8      12.8
   24            0.39-0.47           3.8      26.3   0.43-0.48    3.6     32.0          0.39-0.46             2.4      14.1


IGARSS 2012, Munich, Germany                                             Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                         Chinese Academy of Sciences
                                                                                                        (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Assessment by FOM




IGARSS 2012, Munich, Germany                           Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                       Chinese Academy of Sciences
                                                                                      (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                Progresses of CFOSAT/SCAT
• 2010.04 PDR of SCAT
• 2010.12 Detailed design review
• 2011.07 Delivery of electrical models (except antenna
  subsystem) and satellite electrical performance test
      – System specifications, interface compatibility confirmed
•    2011.11             Delivery of mechanical and thermal models
•    2011.12             Satellite mechanical test
•    2012.02             Satellite thermal test
•    2012.05             RF compatibility test
•    2012.07             Onboard full operation mode test

IGARSS 2012, Munich, Germany                       Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                   Chinese Academy of Sciences
                                                                                  (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                           RFC test and SCAT integrated test

                                                            160
                                                                                                                              定标
                                                                                                                              回波
                                                            140



                                                            120


                                            Amplitude(dB)
                                                            100



                                                            80



                                                            60



                                                            40
                                                             -750   -562.5   -375   -187.5     0     187.5       375     562.5       750
                                                                                        Frequency (KHz)


IGARSS 2012, Munich, Germany                                                           Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                                                       Chinese Academy of Sciences
                                                                                                                      (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Summary
• Design and performance of CFOSAT SCAT is presented:
      – When U<4m/s, SCAT/CFOSAT cannot provide useful wind
        retrieval due to its low SNR;
      – For U=4~8m/s, SCAT/CFOSAT can provide wind retrieval
        similar to QSCAT only within swath of 800km;
      – For U>8m/s, SCAT/CFOSAT can provide better wind
        retrieval with its designed swath of 1000km, compared
        with QSCAT;
      – For U>16m/s, the advantage of SCAT/CFOSAT become
        obvious, due to its more number of looks.
• Development of SCAT on time for the scheduled launch
  in 2014.

IGARSS 2012, Munich, Germany                     Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                 Chinese Academy of Sciences
                                                                                (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences


                                            Further to do…
• New quality control for sigma-0 measurement
  with more number of looks and lower SNR;
• Development of retrieval making use of increased
  number of looks;
• Evaluation of rain effect, compared with pencil
  beam system like QSCAT;
• Calibration for rotating fan beam system:
      – In-orbit antenna pattern calibration;
      – In-orbit possible azimuth-dependent antenna gain
        variation due to rotary joint.
IGARSS 2012, Munich, Germany                         Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                                     Chinese Academy of Sciences
                                                                                    (MiRS, CAS)
National Space Science Center
            Chinese Academy of Sciences




                   Thanks for your attentions!




IGARSS 2012, Munich, Germany                Key Laboratory of Microwave Remote Sensing
July 22-27, 2012                                            Chinese Academy of Sciences
                                                                           (MiRS, CAS)

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PROGRESSES OF DEVELOPMENT OF CFOSAT SCATTEROMETER

  • 1. National Space Science Center Chinese Academy of Sciences PROGRESSES OF DEVELOPMENT OF CFOSAT SCATTEROMETER Xiaolong Dong, Di Zhu CAS Key Laboratory of Microwave Remote Sensing National Space Science Center, CAS PO Box 8701, Beijing, China dongxiaolong@mirslab.cn, zhudi@mirslab.cn IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 2. National Space Science Center Chinese Academy of Sciences Outline of the Presentation • Introduction to the Mission • Specifications of SCAT • Description of SCAT system • Simulation of SCAT system performances • Progresses • Summary IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 3. National Space Science Center Chinese Academy of Sciences • Two payloads: CFOSAT Mission – SWIM (Sea Wave Investigation and Monitoring by satellite) • A Ku-band real aperture radar for • CFOSAT: Chinese French Oceanography measurement of directional ocean wave spectra; SATellie – SCAT (SCATterometer) • Launch plan: 2014 • A Ku-band rotating fan-beam radar • Mission Objectives: scatterometer for measurement of monitoring the wind and waves at the ocean ocean surface wind vector. surface at the global scale in order to improve: – The wind and wave forecast for marine meteorology (including severe events) – the ocean dynamics modeling and prediction, – our knowledge of climate variability – fundamental knowledge on surface processes linked to wind and waves IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 4. National Space Science Center Chinese Academy of Sciences Mission-measurement requirements • Joint measurement of ocean surface wind vector and sea-state parameters from radar – Both wind vector and wave parameters can be measured using active micro-wave remote sensing (heritage of altimeter, sactterometer and SAR missions, and airborne radar measurements) – Wind vector => optimal configuration at medium incidence angle (20-50°) – Wave spectra => optimal configuration at low incidence angle (< 15°) • CFOSAT mission with two payloads – SWIM: wave scatterometer: multi-beam Ku-Band radar at low incidence – SCAT: wind scatteromer: Fan beam Ku-Band radar at medium incidence IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing 4 July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS) 4
  • 5. National Space Science Center Chinese Academy of Sciences Mission-Wind Vector Payload -SCAT • A Ku-band rotating fan-beam radar scatterometer (Ku-RFSCAT) for sea surface wind vector retrieval by measurement of the sea surface backscattering coefficient. Rotating fan-beam antenna • Adapted to the platform constraints (small size); • 2 fan beams (HH & VV) cover incident Nadir Point angles from 26 degree to 46 degree from nadir • scanned with a rotation speed of around footprint 3.5 rpm. • For each of the ground resolution cells, more than four looking angles can be obtained to retrieval wind vector information. IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 5 Chinese Academy of Sciences (MiRS, CAS)
  • 6. National Space Science Center Chinese Academy of Sciences Characteristics of CFOSAT SCAT • Wide swath by rotating of beam; – Decided by outer edge of incident angle of beam • More number of azimuth look angles by overlap of beam; – Decided by flying speed, rotating speed and beamwidth • NRCS/sigma 0 dependent on antenna beam; – Decided by local antenna gain along elevation • Single antenna for all azimuth directions; – No inter-beam balance required – But azimuth fluctuation may exist due to rotating mechanism IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 7. National Space Science Center Chinese Academy of Sciences Azimuth look angle combinations for surface resolution cells Overlap between adjacent scanns for large number of azimuth view for each pixel. Dual polarization is used Surface resolution cell 1 to improve retrieval of outer and center part of the swath Track of nadir porints Surface resolution cell 2 IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 8. National Space Science Center Chinese Academy of Sciences Specifications for SCAT • Objectives: – Measurement of global surface sigma 0 – Retrieval of global ocean surface wind vector • Data requirements – Swath width: >1000km – Surface resolution: 50km (standard); 25km (goal) – Data quality (at 50km resolution) – ° precision: • 1.0dB for wind speed 4~6m/s • 0.5dB for wind speed 6~24m/s – Wind speed: 2m/s or 10% @ 4~25m/s – Wind direction: 20deg @ 360deg for most part of the swath • Life time: 3yrs IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 9. National Space Science Center Chinese Academy of Sciences Specifications of SCAT Ku-RFSCAT Parameters Antenna Spinning rate : 3.5 rpm Polarization: VV, HH PRF/channel: 75 Hz/channel Pulse peak power (Pt): 120 W Pulse bandwidth (B): 0.5 MHz Pulse duration (τp): 1.3 ms Swath width: 1000 km Receive gate length(Tg): 2.82 ms Receive gate delay: 3.74 ms Inclination: 97.5 deg IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 10. National Space Science Center Chinese Academy of Sciences Description of SCAT system • System overview • Choice of system type • Operation mode • System configuration • Key parameters IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 11. National Space Science Center Chinese Academy of Sciences System overview • Ku-band rotating fan-beam scatterometer – Platform dimension – Technology heritage – Available GMFs • Long LMF pulse with de-ramp pulse compression – TX: 1.35ms – RX: 2.72 ms • Digital I-Q receiver with on-board pulse compression processing and resolution cell regrouping • TX/RX channel except antenna and switch matrix identical primary/backup design to ensure liability IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 12. National Space Science Center Chinese Academy of Sciences Choice of system type -Why rotating fan beam? • Why rotating beam? • Why rotating fan beam? – Overlap of surface coverage with – Lower rotating speed to ensure SWIM is requirement, nadir gap life time of rotating mechanism; should be avoided. – Multiple incident angles for – Deployment of multiple fan-beam better wind direction retrieval; antenna is not allowed due to – Large incident angle ranges platform capability. (20~46°) for investigation of – Large swath at a relatively low ocean surface scattering orbit (~500km) requires scanning. characteristics, by compensating with SWIM (0~10°) IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 13. National Space Science Center Chinese Academy of Sciences Other constraints • Antenna dimension: <1.2m • Available Pulsed Ku-TWTA: <140W • Available TWTA PRF: >150Hz • Data rate: <220kpbs • Rotating speed and mechanism lifetime IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 14. National Space Science Center Chinese Academy of Sciences Operation mode • Normal mode: dual polarization with rotation; • Test/cal mode: – raw waveform with lower PRF; – Including both rotating mode and fixed pointing mode; • Single polarization mode IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 15. National Space Science Center Chinese Academy of Sciences System configuration • Antenna subsystem • Power amplifier subsystem – Antenna and feeding network; – TWT and EPC – Scanning mechanism; • Digital subsystem – Servo controller; – Signal generator; • RF subsystem – System controller; – Switch matrix; – Signal processor; – RF receiver; – Communication controller; • RX/TX electronics subsystem • Secondary power supply subsystem – IF receiver; – DC-DC power converter; – Frequency synthesizers; – TC/TM module – TX up-converter • WG & cable assembly IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 16. National Space Science Center Chinese Academy of Sciences System Diagram IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 17. National Space Science Center Chinese Academy of Sciences System configuration • Interface with structure subsystem – Antenna and part of the servo mechanism installed outside the satellite; – Other equipments installed inside the satelltie IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 18. Basic radar parameters Parameter Specifications Frequency 13.256GHz Signal bandwidth 0.5MHz Internal calibration precision Better than 0.15dB Receiver NF ≤2.0dB Insertion loss of TX channel ≤1.5dB Insertion loss of RX channel ≤3.0dB Transmitting power (peak) 120W Pulse width 1.35ms PRF 2×75=150Hz EUMETSAT/ESA Scatterometer Science Conference 2011 April 11-13, Darmstadt, Germany
  • 19. National Space Science Center Chinese Academy of Sciences Optimization of radar parameters • Optimization: trade-off between SNR, measurement samples of each look and number of looks. maximization of wind vector retrieval performance – Surface resolution – Signal bandwidth – Rotating speed IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 20. National Space Science Center Chinese Academy of Sciences Resolution in azimuth direction & azimuth beam-width • Fan beamlower gainantenna as long as possible • Decided by antenna beamwidth • Limited by satellite dimension: ≤1.2m • Beamwidth ~1.1 deg resolution in azimuth direction: 10.5~14.5km IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 21. Design of rotating speed • Trade-off between independent sigma 0measuremrent samples for single look and number of looks • Optimization of 3.5rpm EUMETSAT/ESA Scatterometer Science Conference 2011 April 11-13, Darmstadt, Germany
  • 22. National Space Science Center Chinese Academy of Sciences Resolution in elevation direction & signal bandwidth • Low SNR due to low antenna gain • Bandwidth 0.5MHz resolution:380~650m • On-board non-coherent re- grouping to improve sigma 0 precision resolution of 5km IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 23. National Space Science Center Chinese Academy of Sciences Onboard processing • Reduce data rate to ~220kbps • Downlink data resolution: ~10km(az) × 5km(el) – (original resolution: 10km(az) × (<1km(el)) • Signal+noise processing & noise-only processing IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 24. National Space Science Center Chinese Academy of Sciences Internal Calibration Loop P1 K1 C1 LPF1 P31 P21 Circulator TWTA P22 P32 K6 C2 K2 D K3 K5 A Ns LPF2 K4 P31 P32 Compositions: •C1,C2:directional couplers Ports: •K1,K2,K3,K4:ferrite switches •P1: BJ-140 to TWTA •K5,K6:mechanical switches •P2: BJ-140 to antennas •LPF1/2:EMC filters •P3: BJ-140 to RF receiver •D: power monitoring detector •Ns:internal noise source IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 25. National Space Science Center Chinese Academy of Sciences Simulations of system performances • Simulation model • Simulation of precision • Simulation of wind vector retrieval performance IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 26. National Space Science Center Chinese Academy of Sciences Simulation model IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 27. National Space Science Center Chinese Academy of Sciences Simulation of ° precision • Modeling 2 G2  Pr Pt dA SNR SNR  – Radar equation 3 4 L 4 A R Pr where: N – SNR P 120W 50.8dBm t 1 2 G2  Pt dA – ° precision 3 2.263cm 16.5dB kBT 4 L A R4 L 3.5dB (insturment loss) 2 2  P true 1 1 1 1 Kp  1  1  P true Neff SNR true Nnoise SNR true Kp(dB) 10log 1 Kp IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 28. National Space Science Center Chinese Academy of Sciences • Statistics: number of looks (left) number of independent samples (right) IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 29. National Space Science Center Chinese Academy of Sciences SNR distribution U=4m/s U=8m/s IGARSS 2012, Munich, Germany U=16m/s U=24m/s Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 30. National Space Science Center Chinese Academy of Sciences Kp distribution (25km) U=4m/s U=8m/s IGARSS 2012, Munich, Germany U=16m/s U=24m/s Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 31. National Space Science Center Chinese Academy of Sciences Simulation of wind retrieval • Only °data with precision better than 1.0dB will be used for wind retrieval; • Standard MLE method and NSCAT GMF are used for simulation; • Median filter algorithm for wind direction ambiguity removal • 2 kinds of wind field simulated – Spatially correlated parallel wind field and circular wind field – Random wind field IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 32. National Space Science Center Chinese Academy of Sciences Parallel and circular wind field (U~[2,24]) IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 33. National Space Science Center Chinese Academy of Sciences Retrieval performance of parallel wind field U Qe(m/s)-U QRMS(m/s)-U Qe (o)-phi QRMS (o)-phi 4 0.43 0.65 51.5 65.9 6 0.45 0.66 15.9 22.3 8 0.55 0.76 10.9 16.5 10 0.68 0.93 10.1 15.4 12 0.83 1.13 10.2 15.6 14 0.99 1.33 10.3 15.7 16 1.17 1.57 10.8 16.3 18 1.38 1.83 11.3 17.0 20 1.60 2.12 12.1 18.1 22 1.86 2.43 12.9 19.1 24 2.13 2.75 13.4 19.8 IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 34. National Space Science Center Chinese Academy of Sciences Retrieval performance of circular wind field U Qe(m/s)-U QRMS(m/s)-U Qe (o)-phi QRMS (o)-phi 4 0.44 0.68 39.1 51.9 6 0.46 0.68 15.6 22.3 8 0.55 0.77 10.9 16.6 10 0.69 0.95 10.2 15.7 12 0.86 1.17 10.4 16.0 14 1.02 1.38 10.6 16.3 16 1.22 1.62 11.1 16.9 18 1.44 1.90 11.8 17.8 20 1.68 2.20 12.7 19.0 22 1.93 2.51 13.5 20.0 24 2.19 2.83 14.0 20.7 IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 35. National Space Science Center Chinese Academy of Sciences FOM varying with wind speed IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 36. National Space Science Center Chinese Academy of Sciences Random wind field • Parallel wind field simulated • Wind speed range: 4~24m/s • Wind direction search interval: 10deg • 25km WVC resolution IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 37. National Space Science Center Chinese Academy of Sciences U=4m/s U=8m/s IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 38. National Space Science Center Chinese Academy of Sciences U=16m/s U=12m/s IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 39. National Space Science Center Chinese Academy of Sciences U=24m/s U=20m/s IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 40. National Space Science Center Chinese Academy of Sciences Wind vector retrieval performance RMS of wind speed RMS of wind direction Input wind speed (m/s) (o) 4 0.7 35.5 6 0.7 22.3 8 0.8 16.6 10 1.0 15.7 12 1.2 16.0 14 1.4 16.3 16 1.6 16.9 18 1.9 17.8 20 2.2 19.0 22 2.5 20.0 24 2.8 20.7 IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 41. National Space Science Center Chinese Academy of Sciences Retrieval performance Near nadir Far range within footprint Near range within footprint (-100~+100) (>400km) (100~400km) U(m/s) 0 U phi 0 U phi 0 U phi (dB) (m/s) ( ) (dB) (m/s) ( ) (dB) (m/s) ( ) 4 0.89-1.79 0.4 44.1 1.43-3.07 1.1 44.7 0.66-2.07 0.4 31.8 8 0.46-0.66 0.9 24.2 0.51-1.01 1.3 26.9 0.44-0.74 0.6 11.0 12 0.41-0.53 1.2 22.7 0.45-0.63 1.8 26.6 0.41-0.54 0.9 10.4 16 0.40-0.49 2.1 22.7 0.44-0.54 2.2 27.6 0.40-0.49 1.3 11.3 20 0.40-0.48 2.9 24.8 0.43-0.50 2.9 30.1 0.40-0.47 1.8 12.8 24 0.39-0.47 3.8 26.3 0.43-0.48 3.6 32.0 0.39-0.46 2.4 14.1 IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 42. National Space Science Center Chinese Academy of Sciences Assessment by FOM IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 43. National Space Science Center Chinese Academy of Sciences Progresses of CFOSAT/SCAT • 2010.04 PDR of SCAT • 2010.12 Detailed design review • 2011.07 Delivery of electrical models (except antenna subsystem) and satellite electrical performance test – System specifications, interface compatibility confirmed • 2011.11 Delivery of mechanical and thermal models • 2011.12 Satellite mechanical test • 2012.02 Satellite thermal test • 2012.05 RF compatibility test • 2012.07 Onboard full operation mode test IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 44. National Space Science Center Chinese Academy of Sciences RFC test and SCAT integrated test 160 定标 回波 140 120 Amplitude(dB) 100 80 60 40 -750 -562.5 -375 -187.5 0 187.5 375 562.5 750 Frequency (KHz) IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 45. National Space Science Center Chinese Academy of Sciences Summary • Design and performance of CFOSAT SCAT is presented: – When U<4m/s, SCAT/CFOSAT cannot provide useful wind retrieval due to its low SNR; – For U=4~8m/s, SCAT/CFOSAT can provide wind retrieval similar to QSCAT only within swath of 800km; – For U>8m/s, SCAT/CFOSAT can provide better wind retrieval with its designed swath of 1000km, compared with QSCAT; – For U>16m/s, the advantage of SCAT/CFOSAT become obvious, due to its more number of looks. • Development of SCAT on time for the scheduled launch in 2014. IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 46. National Space Science Center Chinese Academy of Sciences Further to do… • New quality control for sigma-0 measurement with more number of looks and lower SNR; • Development of retrieval making use of increased number of looks; • Evaluation of rain effect, compared with pencil beam system like QSCAT; • Calibration for rotating fan beam system: – In-orbit antenna pattern calibration; – In-orbit possible azimuth-dependent antenna gain variation due to rotary joint. IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)
  • 47. National Space Science Center Chinese Academy of Sciences Thanks for your attentions! IGARSS 2012, Munich, Germany Key Laboratory of Microwave Remote Sensing July 22-27, 2012 Chinese Academy of Sciences (MiRS, CAS)