Satellite Radar Interferometry Contents Part 1 & 2 and its ...

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1 December 6, 2006 1 Satellite Radar Interferometry and its applications Part 1, Radar fundamentals Guest lecture Remote Sensing (GRS-20306) Wageningen University Ramon Hanssen Delft Institute of Earth Observation and Space Systems December 6, 2006 2 Contents Part 1 & 2 Part 1 Radar background and fundamentals Imaging radar, SAR Physics and geometry Resolution Part 2 Interferometry, principles Topography and deformation Accuracy Error sources New processing methodologies: PSI December 6, 2006 3 Radar background/history December 6, 2006 4 December 6, 2006 5 Early ground based radar RAdio Detection and Ranging December 6, 2006 6 Radar mapping of the Moon, Venus, Mars (1946) (1961) (1963) Main parameters: •Distance •Velocity •Intensity Retrograde rotation Venus Improvement of Astronomical unit

Transcript of Satellite Radar Interferometry Contents Part 1 & 2 and its ...

Page 1: Satellite Radar Interferometry Contents Part 1 & 2 and its ...

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December 6, 2006

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Satellite Radar Interferometry and its applicationsPart 1, Radar fundamentals

Guest lecture Remote Sensing (GRS-20306)Wageningen UniversityRamon Hanssen

Delft Institute of Earth Observation and Space Systems

December 6, 2006 2

Contents Part 1 & 2Part 1• Radar background and fundamentals• Imaging radar, SAR• Physics and geometry• ResolutionPart 2• Interferometry, principles• Topography and deformation• Accuracy• Error sources• New processing methodologies: PSI

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Radar background/history

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Early ground based radar

RAdio Detection and Ranging

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Radar mapping of the Moon, Venus, Mars(1946) (1961) (1963)

Main parameters:

•Distance

•Velocity

•Intensity

Retrograde rotation Venus

Improvement of Astronomical unit

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Magellan Synthetic Aperture Radar Mosaic of Venus

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Maat Mons, Venus

Magellan Synthetic Aperture Radar

Radar clinometry, altimeter, and backscatter

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Towards imaging radar

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Optical imagery (false color) versus radar imagery

Delft University, AE

Resolution: 4x20 m

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Physics

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Radio waves, active sensor

Wavelength range is cm-m

24 cm 3 cm5 cm

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Penetration (weather independent)

C b

and

Radar waves penetrate the atmosphere and clouds

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• Landsat optical• Shuttle L-band radar• What do we see?

Sahara desert

Radar penetrates material with a low dielectric constant (dep. on wavelength)

Here about 3 m.

Sahara, NW Sudan (SIR-A)

Physics

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Physics - Scattering

• Scattering is dominated by wavelength-scale structures

• Wavelength shorter: image brighter• Specular and Bragg scattering• Speckle

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SPECULAR

Radar signal return depends on:

•Slope

•Roughness

•Dielectric constant

Scattering

Smooth Rough

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Physics – scattering phase

Imag

inar

y

Real

Radar pixel phase is superposition of near-random scattering elements:

Unpredictable!

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December 6, 2006 1

Geometry

Terminology • Foreshortening, layover, shadow• Why side-looking?• Incidence angle, • Coordinates range, azimuth

December 6, 2006 2

Fore

short

ening

Layo

ver

Shado

w

Geometry Slant range

Ground range

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Geometry

Fore

short

ening

Layo

ver

Shado

w

JERS-1 data (M.Shimada)

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Resolution I: RAR•Real Aperture Radar

•Resolution dependent on antenna dimension/pulse length

•Beam width (half power width) is ratio wavelength over antenna size:

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Antenna dimensions

1.3 m

10 m

Calculate Ground Resolution

C-band λ= ~0.05 m

D=10 m antenna

Beam angle = 5.10-2/10 = 5.10-3 rad

R=850 km

times 8.5.105 = 42.102[m] = 4.2 km

Dλθ =

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antenna

pulse

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antenna

pulse length

pulse repetition

frequency (PRF)

swath

ground range

Slant range

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Improvement of along-track resolution

Synthetic antenna

Physical antenna

Resolution cell

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Improvement in Resolution (Crimea, Ukraine)

Real Aperture Radar Synthetic Aperture Radar

5x14 km pixels 4x20 m pixels

Massonnet and Feigl, 1998

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Resolution II: SAR

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Resolution II (SAR)

• Resolution SAR is inversely proportional with bandwidth

• Azimuth resolution SAR: Half antenna size!

• No influence of satellite height on azimuth resolution SAR image

• Range resolution improvement using chirp waveform

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SAR SLC observationsSLC: Single-Look Complex data

•Single-look: no averaging, finest spatial resolution

•Complex: both real and imaginary (In-phase and quadrature phase) stored

Amplitude PhaseUninterpretable, due to scattering mechanism

Coherent imaging

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End of part 1

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Satellite Radar InterferometryPart 2, InSAR, fundamentals and applications

Guest lecture Remote Sensing, Wageningen University

Ramon Hanssen

Delft Institute of Earth Observation and Space Systems

December 6, 2006 15

Interferometric radar (InSAR)

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Radar Interferometry

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Example in 2D: interferogram

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Range

Expressed as phase (radians)

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Range

Expressed as integer cycles + fractional phase

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Reference phase (flat earth phase)

Ellipsoid

Topography will add variation to the “flat earth phase”

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Phase-range relationship

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Phase-height relationship(Far-field approximation)

Ellipsoid

Topographic phase is (inversely) scaled by the perpendicular baseline!

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Amplitude

Reference phase

Topographic phase

RADAR INTERFEROMETRIC OBSERVATIONS

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Phase and topography

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Baseline dependency, height ambiguity

Bperp 173 m, Bt= 1day Bperp 531 m, Bt= 1 day

H2pi=45m H2pi=16m

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Deformation measurements

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Conventional Interferometry: Bam earthquake 26/12/2003

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Conventional Interferometry: Glacier Dynamics (Svalbard, Spitsbergen)

5 KM

LOS

12 day interferogram

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Satellite radar interferometry• Coseismic interferogram, showing deformation Izmit earthquake

• Every color cycle 7.5 cm horizontal motion

• Showing which segment of fault ruptured

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Mauna Loa, Hawaii• Deformation

(inflation) of the Mauna Loa summit

• Position of the magma chamber better determined

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…Very sensitive to deformation

Subsidence Las Vegas due to ground water extraction

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Phase-deformation relationship

Subsidence ∆z

1 cycle LOS deformation is equal to half the physical wavelength

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Topography and deformation

Ellipsoid

Sensitivity to deformation 1000x higher than for topography

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Quality: Phase variance estimation:Coherence

•Optics equivalent to correlation:

•Estimation of coherence:

}|{|}|{|}{

22

21

*21

yEyEyyE⋅

∑ ∑∑

= =

==N

n

N

nnn

N

nnn

yy

yy

1 12)(

22)(

1

1)(

2)(

1

||||

|||ˆ| γ

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Coherence

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Problems Conventional InSAR• Close satellite orbits required• Sensitive to changing surface backscatter behavior• Sensitive to atmospheric water vapor

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1 day

16618593112Perpendicular baseline (m)

6 years3 years2 years1 yearTemporal baseline

Conclusion:

Conventional InSAR does not work for

•slow deformation, over

•vegetated/wet/changing surfaces,

•in non-arid climate regions

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New processing methodologies

• To resolve the ambiguities• Separate topography and deformation• To detect information in the noise• To estimate/mitigate atmospheric signal• To estimate orbit errors

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Deformationmeasurements:time-seriesapproaches

• Evaluation per point: double-differences

• Opportunistic subsets

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PS principle• Pixels with strong and consistent reflections in

time.• Multi-pass InSAR – time series necessary.• Estimate atmosferic signal:

• Spatially, not temporally correlated.• Independent of baseline. (topography is)

Salt mining Nedmag Veendam

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1992 2004

1992

1992 2004

2004

Formal precision of deformation rate < 1 mm/y

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Interpolated signal

mm/y1992-2004

December 6, 2006 921 Dec 2003

28 May 1992

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Case study Harlingen

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Case study Harlingen

mm/year

Local salt mining resulted in subsidence. The dike segment subsided ~5 cm between 1995 and 2001

1992 1995 2001

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Sluices Kornwerderzand

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Case study Kornwerderzand

mm/year

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mm/year

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Case study Marken

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mm/year

0

NAP

-2

-4

-6Compaction

clay

peat

clay

stones

Settlement of peat layers below Markenisland caused a vertical movement of the dikes of ~10 cm between 1992 and 2001

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Case Study Noordoostpolder

Taken from: www.wikipedia.nl

UrkSchokland

Emmeloord

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‘Zetting’