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[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object], / 13
Outline ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object], / 13
1. PAU-SA Instrument   / 13  PAU-SA in the robotic arm 8 m PAU-RAD PAU-GNSS-R PAU-IR
 / 13  2. Potential improvements for future SMOS’s Parameter MIRAS/SMOS PAU-SA Comments Frequency operation L-band (1400 - 1427 MHz) L-band (1575.42 MHz) L1 of GPS signal Same frequency both Radiometry and GPS Reflectrometry Bandwidth 19 MHz 2.2 MHz Spatial correlation effects negligible Larger   T Arm size 4 m 1.3 m Altitude Global observation, LEO, orbital altitude ground-based - Antenna type Patch antenna with  V & H polarizations  (not simultaneous) Patch antenna with  V & H polarizations (simultaneous) Full-pol (non-sequential) Number of antennas per arm 23 8 +1 (dummy) Improve antenna pattern similarity Number total antennas 69 31 - Antenna spacing 0.875     at 1400 MHz, (21 cm) 0.816    at 1575.42 MHz, (15.5 cm) Increase the alias-free field of view Receiver type single polarization (1 per element) dual polarization (2 per element) Full-pol (non-sequential) Topology of the LO  down-converter Distributed LO  (groups of 6 elements) Centralized reference clock + internal LO generated in each receiver Reduce LO leakage and  correlated offset Quantization 1 bit   (Inside the LICEF ) 8 bits IF sub-sampling   using a external ADC Digital I/Q demodulation Digital Power measurement   Digital LPF  I/Q conversion Analog Digital Elimination quadrature error Frequency response shaped by Analog RF filter Digital low- pass filter Mass reduction,  quasi perfect matching,  no temperature and  aging drifts  Power measurement system (PMS) Analog (Schottky diode) Digital (FPGA) Mass reduction,  Thermal drifts minimized Calibration by Noise Injection Injection of  Distributed noise Injection of  Centralized noise  or PRN signal Simpler calibration. Calibration of non-separable errors Recs’ freq. response estimation Image capabilities Dual-pol or full-pol (sequential) Full-pol (non-sequential) Necessary to GNSS-R applications
3.1. Use of PRN Signals for: FWF determination  / 13  FWF(Y1Y2) ,[object Object],[object Object],[object Object],[object Object],[object Object],Centralized Calibration using: Noise Source or  PRN sequences   SR=0.5 SR=1 SR=5 I. Ramos-Pérez et al., “ Use of Pseudo-Random Noise sequences in  microwave radiometer calibration ”,  MICRORAD 2008   I. Ramos-Pérez et al., “Calibration of Correlation Radiometers Using  Pseudo-Random Noise Signals” Sensors 2009 ISSN 1424-8220
3.2. Use of PRN Signals for: Receiver’s frequency response  / 13  A S PRN +S R2 S PRN +S R1 Correlation of receivers’ output with local replica of PRN signal injected allows individual frequency responses to be measured (amplitude and phase) Using:  PRN sequences
4.1. Inter-calibration time in real-time systems  / 13  Data : PAU-SA instrument Measurement :  τ   =1 s., every 2 min  Off-line Processing    Decimate  to simulate lack of data  ,[object Object],[object Object],[object Object],[object Object],[object Object],INTERPOLATION ERROR: No aliasing Decimation factor 4 (8 min) Conclusion:  Real-time systems require much more often calibration time to avoid estimation errors to propagate and increase rapidly  EKF B ~ 1 mHz T inter-cal max  = 1 / 2·B ~ 4 min If T inter-cal  >  4 min  Aliasing  interpolation phase error  Real-time Processing    Prediction, e.g.  with Extended  Kalman filter (EKF)
4.2. Inter-calibration time in off-line systems: SMOS  / 13  Data : SMOS (L1 level)   Commissioning Phase Measurement :  τ   =1.2 s., every 2 min Decimation Interpolation  with different methods No aliasing     Optimum  inter-calibration time ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],All visibilities (fft interpolation) ,[object Object],[object Object],[object Object],[object Object],Optimum  interpolation B ~ 1.25 mHz T inter-cal max  = 1 / 2·B ~ 7 min If T inter-cal  >  7 min  Aliasing  interpolation phase error
5.1. Preliminary results (i): Impulse response  / 13  FFT  Point Source  : PRN signal (-70 dBm) Moving the Instrument  (no temperature control)   El +/- 10º, +/- 20º   Az +/- 10º, +/- 20º   Pol H Az= 0º El= 0º Pol H Az= +10º El= 0º Pol H Az= +20º El= 0º Pol V Az= 0º El= +10º Pol V Az= 0º El= +20º PRN Signal Rectangular window for visibility samples Antenna  1 PRN Source  1 Instrumen t
5.2. Preliminary results (ii):  Angular resolution  / 13  FFT  Point Source   : PRN signals (-70 dBm) 7 antennas per arm + rectangular window Sources – PAU-SA distance at 10 m Angular resolution   ( ξ , η )  ~  5.7º 2 PRN Signals Rectangular  window PRN Source  1 Antenna  1 PRN Source  2 Antenna   2 Instrumen t Antennas separation at: (Near field) No near-to-far field transformation applied 1 m  2 m  3 m  4 m
5.3. Preliminary results (iii): GPS satellites  / 13  FFT  GPS Signal Rectangular  window UPC location GPS orbit UTC 12:44:03   K UTC 12:22:03   K UTC 12:00:03   K UTC 11:38:03   K
5.4. Preliminary results (iv): GPS satellites  / 13  K
6. Summary ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object], / 13
 / 13  Mr. Isaac Ramos Responsible for the design and  manufacturing of the instrument Thank you!

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TH2_T03_5_PAU-SA_I_Ramos.ppt

  • 1.
  • 2.
  • 3. 1. PAU-SA Instrument / 13 PAU-SA in the robotic arm 8 m PAU-RAD PAU-GNSS-R PAU-IR
  • 4. / 13 2. Potential improvements for future SMOS’s Parameter MIRAS/SMOS PAU-SA Comments Frequency operation L-band (1400 - 1427 MHz) L-band (1575.42 MHz) L1 of GPS signal Same frequency both Radiometry and GPS Reflectrometry Bandwidth 19 MHz 2.2 MHz Spatial correlation effects negligible Larger  T Arm size 4 m 1.3 m Altitude Global observation, LEO, orbital altitude ground-based - Antenna type Patch antenna with V & H polarizations (not simultaneous) Patch antenna with V & H polarizations (simultaneous) Full-pol (non-sequential) Number of antennas per arm 23 8 +1 (dummy) Improve antenna pattern similarity Number total antennas 69 31 - Antenna spacing 0.875  at 1400 MHz, (21 cm) 0.816  at 1575.42 MHz, (15.5 cm) Increase the alias-free field of view Receiver type single polarization (1 per element) dual polarization (2 per element) Full-pol (non-sequential) Topology of the LO down-converter Distributed LO (groups of 6 elements) Centralized reference clock + internal LO generated in each receiver Reduce LO leakage and correlated offset Quantization 1 bit (Inside the LICEF ) 8 bits IF sub-sampling using a external ADC Digital I/Q demodulation Digital Power measurement Digital LPF I/Q conversion Analog Digital Elimination quadrature error Frequency response shaped by Analog RF filter Digital low- pass filter Mass reduction, quasi perfect matching, no temperature and aging drifts Power measurement system (PMS) Analog (Schottky diode) Digital (FPGA) Mass reduction, Thermal drifts minimized Calibration by Noise Injection Injection of Distributed noise Injection of Centralized noise or PRN signal Simpler calibration. Calibration of non-separable errors Recs’ freq. response estimation Image capabilities Dual-pol or full-pol (sequential) Full-pol (non-sequential) Necessary to GNSS-R applications
  • 5.
  • 6. 3.2. Use of PRN Signals for: Receiver’s frequency response / 13 A S PRN +S R2 S PRN +S R1 Correlation of receivers’ output with local replica of PRN signal injected allows individual frequency responses to be measured (amplitude and phase) Using: PRN sequences
  • 7.
  • 8.
  • 9. 5.1. Preliminary results (i): Impulse response / 13 FFT Point Source : PRN signal (-70 dBm) Moving the Instrument (no temperature control) El +/- 10º, +/- 20º Az +/- 10º, +/- 20º Pol H Az= 0º El= 0º Pol H Az= +10º El= 0º Pol H Az= +20º El= 0º Pol V Az= 0º El= +10º Pol V Az= 0º El= +20º PRN Signal Rectangular window for visibility samples Antenna 1 PRN Source 1 Instrumen t
  • 10. 5.2. Preliminary results (ii): Angular resolution / 13 FFT Point Source : PRN signals (-70 dBm) 7 antennas per arm + rectangular window Sources – PAU-SA distance at 10 m Angular resolution  ( ξ , η ) ~ 5.7º 2 PRN Signals Rectangular window PRN Source 1 Antenna 1 PRN Source 2 Antenna 2 Instrumen t Antennas separation at: (Near field) No near-to-far field transformation applied 1 m 2 m 3 m 4 m
  • 11. 5.3. Preliminary results (iii): GPS satellites / 13 FFT GPS Signal Rectangular window UPC location GPS orbit UTC 12:44:03 K UTC 12:22:03 K UTC 12:00:03 K UTC 11:38:03 K
  • 12. 5.4. Preliminary results (iv): GPS satellites / 13 K
  • 13.
  • 14. / 13 Mr. Isaac Ramos Responsible for the design and manufacturing of the instrument Thank you!