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Correction of Ionospheric Distortions in Low Frequency Interferometric SAR Data Jun Su Kim, Pau Prats & Konstantinos P. Papathanassiou Microwave and Radar Institute  German Aerospace Center
SAR imaging through the Earth’s ionosphere ,[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object],[object Object]
Azimuth shift decorrelation ,[object Object],TEC change rate of 5 TECU/100 km Varying ionosphere : Azimuth shift [pixel] : Velocity of piercing point : Pulse repetition frequency : Doppler rate : azimuth distance Satellite orbit
Azimuth shift: result (   comparison) Before After ALOS-PalSAR: Collville, Alaska ,[object Object],Shift FR Contour: Impovement larger than 0.2 ,[object Object],Pauli
Interferometric phase: First order effect ,[object Object],[object Object],[object Object],[object Object],[object Object],Interferograms under ionospheric phases Collville Beaver
Interferometric phase: correction and results - = Original  FR Corrected phase
Combined estimation: principle Mean -> FR  Slant -> shift Varying ionosphere ,[object Object],Coherent length =  L ,[object Object],[object Object],Satellite orbit
Combined estimation: estimation (phase and coherence) ,[object Object],[object Object],FR only Combined Interferometric phase correction Coherence comparison:  a  by 3-ways
Correction using estimated   TEC ,[object Object],[object Object],SLC Decompress  iono Compress SLC’ r iono =0 km r iono =100 km r iono =200 km r iono =300 km
Full band vs. Sub-band az. shift estimation Low Middle High Full Low Middle High
Sub-band Correction scheme 6 sublooks 3 sublooks Full band
Differential az. sub-band interferogram GROUND ORBIT Ionospheric intensity S 1 S 2 S 3
Differential az. sub-band interferogram N=2 ,[object Object],[object Object],[object Object],[object Object],N=9  a estimation
Simulated 6MHz P-band data Without Ionospheric disturbances Coherence-range HH channel SLC Coherence with undisturbed master (N=81) Under Ionospheric disturbances (kp=3, Ckl=50)
Interferometric phase retrieval  (kp=3, Ckl=50) Ionospheric phase screen Coherence as a function of range Nr of Looks =3 A = 3,000 m Nr of Looks =33 A = 300 m Nr of Looks =10 A = 1,000 m Nr of Looks =100 A = 100 m
Interferometric phase retrieval (Far Range) Ionospheric phase screen Nr of Looks =3 A = 3,000 m Nr of Looks =33 A = 300 m Nr of Looks =10 A = 1,000 m Nr of Looks =100 A = 100 m
Conclusion Air-borne motion compensation method can be applied. Combination of Az shift and   FR gives better   TEC estimation. Azimuth shift can be corrected for slow ionospheric variations. Azimuth  full band  approach Performance increases with increasing number of looks (i.e. degreasing azimuth apperture) on the cost of spatial resolution. Sub-band inter-interferogram is well coincidence with direct shift estimation Azimuth shift is compensated also in sub-bands.  Azimuth  sub-band  approach Sub-band approach always give finer structure of the ionosphere
Correction of Ionospheric Distortions in Low Frequency Interferometric SAR Data Jun Su Kim, Pau Prats & Konstantinos P. Papathanassiou Microwave and Radar Institute  German Aerospace Center

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Correction of ionospheric distortions in low frequency interferometric SAR data_final.ppt

  • 1. Correction of Ionospheric Distortions in Low Frequency Interferometric SAR Data Jun Su Kim, Pau Prats & Konstantinos P. Papathanassiou Microwave and Radar Institute German Aerospace Center
  • 2.
  • 3.
  • 4.
  • 5.
  • 6. Interferometric phase: correction and results - = Original  FR Corrected phase
  • 7.
  • 8.
  • 9.
  • 10. Full band vs. Sub-band az. shift estimation Low Middle High Full Low Middle High
  • 11. Sub-band Correction scheme 6 sublooks 3 sublooks Full band
  • 12. Differential az. sub-band interferogram GROUND ORBIT Ionospheric intensity S 1 S 2 S 3
  • 13.
  • 14. Simulated 6MHz P-band data Without Ionospheric disturbances Coherence-range HH channel SLC Coherence with undisturbed master (N=81) Under Ionospheric disturbances (kp=3, Ckl=50)
  • 15. Interferometric phase retrieval (kp=3, Ckl=50) Ionospheric phase screen Coherence as a function of range Nr of Looks =3 A = 3,000 m Nr of Looks =33 A = 300 m Nr of Looks =10 A = 1,000 m Nr of Looks =100 A = 100 m
  • 16. Interferometric phase retrieval (Far Range) Ionospheric phase screen Nr of Looks =3 A = 3,000 m Nr of Looks =33 A = 300 m Nr of Looks =10 A = 1,000 m Nr of Looks =100 A = 100 m
  • 17. Conclusion Air-borne motion compensation method can be applied. Combination of Az shift and  FR gives better  TEC estimation. Azimuth shift can be corrected for slow ionospheric variations. Azimuth full band approach Performance increases with increasing number of looks (i.e. degreasing azimuth apperture) on the cost of spatial resolution. Sub-band inter-interferogram is well coincidence with direct shift estimation Azimuth shift is compensated also in sub-bands. Azimuth sub-band approach Sub-band approach always give finer structure of the ionosphere
  • 18. Correction of Ionospheric Distortions in Low Frequency Interferometric SAR Data Jun Su Kim, Pau Prats & Konstantinos P. Papathanassiou Microwave and Radar Institute German Aerospace Center