2010 igarss cjones mocomp poster reva - nasa ·...

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ADVANCED MOTION COMPENSATION FOR AIRBORNE PLATFORMS: APPLICATION TO UAVSAR Cathleen Jones, Scott Hensley, Thierry Michel, Ron Muellershoen Jet Propulsion Laboratory, California Institute of Technology Copyright 2010 California Institute of Technology. Government sponsorship acknowledged. Topography and AzimuthDependent Motion Compensation Effect on UAVSAR Repeat Track Interferometric Results http://uavsar.jpl.nasa.gov Flight track is more difficult to repeat in an aircraft: Requires knowledge of aircraft motion and position to ~few cm level. (SOLUTION: combine INU and differential DGPS measurement for increased position and orientation accuracy) Large repeat track baselines lead to decorrelation. (SOLUTION: precision control of flight track to ±5 meters) Residual motion smaller than the detected motion must be estimated to achieve sub-centimeter deformation accuracy. (SOLUTION: advanced processing algorithms to estimate residuals from image offsets between repeat tracks) Aircraft attitude angles depends upon variable flight conditions: Variable wind conditions can cause the aircraft yaw angle to change on a timescale smaller than the synthetic aperture formation time during a flight line. (SOLUTION: adaptively steer antenna during a flight line to compensate yaw variation) Both yaw and pitch can be different between repeat tracks because of wind, fuel load, velocity, and initial conditions. (SOLUTION: Adaptive steering to planned flight track, plus process data to the doppler angle that maximizes spectral overlap between the data from the different tracks) Motion Compensation Challenges for an Airborne Platform Additional Challenges for High Precision Repeat Track Interferometry Traditional mocomp ignore the effects of surface topography and finite beam width: Residual Motion Estimation track2 track1 Regular Mocomp Reference Surface Actual Terrain ρ2 ρ1 ρ2 ρ1 B Δρ = λΔφ 4π = Δρ surface + Δρ motion Δρ motion B ρ ρ ˆ l ρ ρ Terrain and attitude angle differences both cause an error in track alignment, and affect both B and Î. Errors in the baseline, B, or the look direction, Î, lead to errors in the interferometric phase and hence to the derived deformation. The advanced mocomp algorithm is implemented after standard motion compensation and before azimuth compression. The data from a single patch is separated into blocks to account for fast attitude changes. The data is Fourier transformed in the azimuth direction to obtain the doppler angle-dependence. The azimuth angle is determined from the frequency of each bin in the inverse FFT azimuth frequency spectrum. The terrain height is determined from the intersection of the doppler cone, the surface ellipsoid and the slant range sphere, iterating to match the DEM height at the intersection point. The interferometric phase correction is calculated with the new look direction and baseline. range azimuth -> block i One patch, in time domain, following presum & standard mocomp azimuth time domain bin j azimuth frequency domain Az FFT θj = sin 1 f j λ 2 Doppler (azimuth) angle Az iFFT Az FFT ×e iΔφmotion range azimuth -> block i azimuth time domain bin j azimuth frequency domain Az iFFT One patch, in time domain, after advanced mocomp Process Flow Regular Mocomp Advanced Mocomp 2π radian phase wrap Repeat Track Interferograms Mount Saint Helens 3/24/2008 4 hr repeat interval Range Azimuth Before After The unknown motion residuals that remain after processing with the advanced motion compensation algorithm are estimated from the measured offsets in range and azimuth between the images for the two tracks. Δs ˆ v ˆ s ( ) sin α steer ( B ˆ l ) ( B ˆ n Doppler ) + ρ ˆ l c B c s + ρ ˆ l h B h s ˆ v ˆ n Doppler sin α steer v ˆ l ) s = along track (azimuth) c = across track h = vertical

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Page 1: 2010 IGARSS CJones Mocomp Poster RevA - NASA · ADVANCED’MOTION’COMPENSATION’FORAIRBORNE’PLATFORMS:’ APPLICATION’TO’UAVSAR Cathleen(Jones,(Scott(Hensley,(ThierryMichel,(Ron(Muellershoen

ADVANCED  MOTION  COMPENSATION  FOR  AIRBORNE  PLATFORMS:  APPLICATION  TO  UAVSAR  

Cathleen  Jones,  Scott  Hensley,  Thierry  Michel,  Ron  Muellershoen  Jet  Propulsion  Laboratory,  California  Institute  of  Technology  

Copyright 2010 California Institute of Technology. Government sponsorship acknowledged.

Topography  and  Azimuth-­‐Dependent  Motion  Compensation   Effect  on  UAVSAR  Repeat  Track  Interferometric  Results  

http://uavsar.jpl.nasa.gov

Flight track is more difficult to repeat in an aircraft:  Requires knowledge of aircraft motion and position to ~few cm level. (SOLUTION: combine INU and differential DGPS measurement for increased position and orientation accuracy)  Large repeat track baselines lead to decorrelation. (SOLUTION: precision control of flight track to ±5 meters)  Residual motion smaller than the detected motion must be estimated to achieve sub-centimeter deformation accuracy. (SOLUTION: advanced processing algorithms to estimate residuals from image offsets between repeat tracks)

Aircraft attitude angles depends upon variable flight conditions:  Variable wind conditions can cause the aircraft yaw angle to change on a timescale smaller than the synthetic aperture formation time during a flight line. (SOLUTION: adaptively steer antenna during a flight line to compensate yaw variation)  Both yaw and pitch can be different between repeat tracks because of wind, fuel load, velocity, and initial conditions. (SOLUTION: Adaptive steering to planned flight track, plus process data to the doppler angle that maximizes spectral overlap between the data from the different tracks)

Motion Compensation Challenges for

an Airborne Platform

Additional Challenges for High Precision Repeat Track Interferometry Traditional mocomp ignore the effects of surface topography and finite beam width:

Residual  Motion  Estimation  €

track2

track1

Regular Mocomp Reference Surface

Actual Terrain

ρ 2

ʹ′ ρ 1

ʹ′ ρ 2

ρ 1

B

Δρ =λΔφ4π

= Δρsurface +Δρmotion

Δρmotion ≈ B • ρ ρ

ˆ l ≡ ρ ρ

Terrain and attitude angle differences both cause an error in track alignment, and affect both B and Î. Errors in the baseline, B, or the look direction, Î, lead to errors in the interferometric phase and hence to the derived deformation.

  The advanced mocomp algorithm is implemented after standard motion compensation and before azimuth compression.

  The data from a single patch is separated into blocks to account for fast attitude changes.

  The data is Fourier transformed in the azimuth direction to obtain the doppler angle-dependence. The azimuth angle is determined from the frequency of each bin in the inverse FFT azimuth frequency spectrum.

  The terrain height is determined from the intersection of the doppler cone, the surface ellipsoid and the slant range sphere, iterating to match the DEM height at the intersection point.

  The interferometric phase correction is calculated with the new look direction and baseline.

range

azimuth ->

block i

One patch, in time domain, following presum & standard mocomp

azimuth time

domain

bin j

azimuth frequency domain

Az FFT

θ j = sin−1f jλ2

⎝ ⎜

⎠ ⎟

Doppler (azimuth) angle

Az iFFT Az FFT

×eiΔφmotion

range

azimuth ->

block i

azimuth time

domain

bin j

azimuth frequency domain

Az iFFT

One patch, in time domain, after advanced mocomp

Pro

cess

Flo

w

Regular Mocomp Advanced Mocomp

2π radian phase wrap

Repeat Track Interferograms

Mount Saint Helens 3/24/2008

4 hr repeat interval

Range

Azimuth

Before

After

The unknown motion residuals that remain after processing with the advanced motion compensation algorithm are estimated from the measured offsets in range and azimuth between the images for the two tracks.

Δs ≈ ˆ v • ˆ s ( )sinαsteer(

B • ˆ l )− (

B • ˆ n Doppler )+ρ ˆ l c

∂Bc

∂s+ρ ˆ l h

∂Bh

∂sˆ v • ˆ n Doppler − sinαsteer( ˆ v • ˆ l )

⎜ ⎜ ⎜

⎟ ⎟ ⎟

s = along track (azimuth)c = across trackh = vertical