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School of Earth and Environment Institute of Geophysics and Tectonics Robust corrections for topographically-correlated atmospheric noise in InSAR data from large deforming regions By David Bekaert Andy Hooper, Tim Wright and Richard Walters

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School of Earth and Environment

Institute of Geophysics and Tectonics

Robust corrections for topographically-correlated atmospheric noise in InSAR data from large deforming regions

By David Bekaert

Andy Hooper, Tim Wright and Richard Walters

School of Earth and Environment Why a tropospheric correction for InSAR?

Tectonic

Over 9 months

100 km

cm

-10 13.5

To extract smaller deformation signals

School of Earth and Environment

To extract smaller deformation signals

Tropospheric delays can reach up to 15 cm

With the tropospheric delay a superposition of

- Short wavelength turbulent component

- Topography correlated component

- Long wavelength component

Troposphere

1 interferogram

(ti –tj)

Tectonic

Over 9 months

100 km

cm

-10 13.5

Why a tropospheric correction for InSAR?

School of Earth and Environment

Auxiliary information (e.g.): Limitations

• GPS

• Weather models

• Spectrometer data

Station distribution

Accuracy and resolution

Cloud cover and temporal sampling

Tropospheric corrections for an interferogram

School of Earth and Environment

Auxiliary information (e.g.): Limitations

• GPS

• Weather models

• Spectrometer data

Interferometric phase

• Linear estimation (non-deforming region or band filtering)

Station distribution

Accuracy and resolution

Cloud cover and temporal sampling

Assumes a laterally uniform troposphere

isolines

Δφtropo =Kuniform ⋅ h +Const

Tropospheric corrections for an interferogram

School of Earth and Environment

A linear correction can work in small regions Interferogram

Tropo

GPS

InSAR and GPS data property of IGN

Linear est

isolines

Δφtropo =Kuniform ⋅ h +Const

A laterally uniform troposphere

School of Earth and Environment

However

• Spatial variation of troposphere

est: Spectrometer & Linear

isolines

+ +

- +

A linear correction can work in small regions

Δφtropo =Kuniform ⋅ h +Const

A spatially varying troposphere

Topography

School of Earth and Environment

Allowing for spatial variation

Interferogram (Δɸ)Why not estimate a linear function locally?

Δφtropo =Kuniform ⋅ h +Const

-9.75 rad 9.97A spatially varying troposphere

School of Earth and Environment

Δφtropo =Kuniform ⋅ h +Const

-9.75 rad 9.97A spatially varying troposphere

Why not estimate a linear function locally?

Does not work as:

Const is also spatially-varying and

cannot be estimated from original phase!

Interferogram (Δɸ)

School of Earth and Environment

Δφtropo =Kspatial ⋅ h0 − h( )α

Δφtropo =Kuniform ⋅ h +Const

-9.75 rad 9.97

We propose a power-law relationship

that can be estimated locally

A spatially varying troposphere

Why not estimate a linear function locally?

Does not work as:

Const is also spatially-varying and

cannot be estimated from original phase!

Interferogram (Δɸ)

School of Earth and Environment

Δφtropo =Kspatial ⋅ h0 − h( )α

With h0 the lowest height at which the relative

tropospheric delays ~0

• 7-14 km from balloon sounding

Sounding data provided by the University of Wyoming

Allowing for spatial variation

School of Earth and Environment

Allowing for spatial variation

Δφtropo =Kspatial ⋅ h0 − h( )α

With h0 the lowest height at which the relative

tropospheric delays ~0

• 7-14 km from balloon sounding

With α a power-law describing the decay of

the tropospheric delay

• 1.3-2 from balloon sounding data

Allowing for spatial variation

Sounding data provided by the University of Wyoming

School of Earth and Environment Power-law example

Δφ =Kspatial ⋅ h0 − h( )α+ Δφdefo + ...

-9.75 rad 9.97

Interferogram (Δɸ)

School of Earth and Environment Power-law example

-9.75 rad 9.97

Δφband≈ Kspatial ⋅ h0 − h( )

α

band

Band filtered: phase (Δɸband) & topography (h0-h)αband

(Y. Lin et al., 2010, G3) for a linear approach

Interferogram (Δɸ)

School of Earth and Environment Power-law example

Δφband≈ Kspatial ⋅ h0 − h( )

α

band

Band filtered: phase (Δɸband) & topography (h0-h)αband

(Y. Lin et al., 2010, G3) for a linear approach

School of Earth and Environment Power-law example

Band filtered: phase (Δɸband) & topography (h0-h)αband €

Δφband≈ Kspatial ⋅ h0 − h( )

α

band

For each window:estimate Kspatial

(Y. Lin et al., 2010, G3) for a linear approach

Anti-correlated!

School of Earth and Environment Power-law example

Δφband≈ Kspatial ⋅ h0 − h( )

α

band

Band filtered: phase (Δɸband) & topography (h0-h)αband

For each window:estimate Kspatial

(Y. Lin et al., 2010, G3) for a linear approach

Anti-correlated!

School of Earth and Environment

Original phase (Δɸ)

Power-law example

Band filtered: phase (Δɸband) & topography (h0-h)αband Tropo variability (Kspatial) €

Δφband≈ Kspatial ⋅ h0 − h( )

α

band

rad/mα -1.1e-6 9.8e-5

School of Earth and Environment

Original phase (Δɸ)

Power-law example

Band filtered: phase (Δɸband) & topography (h-h0)αband Tropo variability (Kspatial) €

Δφtropo =Kspatial ⋅ h0 − h( )α

Topography (h0-h)α

-1.1e-6 9.8e-5rad/mα

-9.75 rad 9.97

Power-law est (Δɸtropo)

4.7e4 2.4e51/mα

School of Earth and Environment

Allowing for spatial variation-9.75 rad 9.97 -9.75 rad 9.97 -9.75 rad 9.97

Original phase (Δɸ) Power-law est (Δɸtropo) Spectrometer est (Δɸtropo)

Power-law example

School of Earth and Environment

Regions:

• El Hierro (Canary Island)

- GPS

- Weather model

- Uniform correction

- Non-uniform correction

• Guerrero (Mexico)

- MERIS spectrometer

- Weather model

- Uniform correction

- Non-uniform correction

Case study regions

School of Earth and Environment

-11.2 rad 10.7

Interferograms(original)

El Hierro

School of Earth and Environment

WRF(weather model)

El Hierro

-11.2 rad 10.7

Interferograms(original)

School of Earth and Environment

WRF(weather model)

El Hierro

-11.2 rad 10.7

Interferograms(original)

School of Earth and Environment

WRF(weather model)

Linear(uniform)

El Hierro

-11.2 rad 10.7

Interferograms(original)

School of Earth and Environment

WRF (weather model)

Linear(uniform)

Power-law(spatial var)

El Hierro

-11.2 rad 10.7

Interferograms(original)

School of Earth and Environment El Hierro quantification

ERA-I run at 75 km resolution WRF run at 3 km resolution

School of Earth and Environment

MERIS MERIS

Mexico-9.75 rad 9.97

School of Earth and Environment

MERIS MERIS

Clouds

Mexico-9.75 rad 9.97

School of Earth and Environment

MERIS ERA-I MERIS ERA-I

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I MERIS ERA-I

Misfit near coast

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I Linear MERIS ERA-I Linear

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I Linear MERIS ERA-I Linear

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I Linear Power-law MERIS ERA-I Linear Power-law

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I Linear Power-law MERIS ERA-I Linear Power-law

Mexico-9.75 rad 9.97(Weather model)

School of Earth and Environment

MERIS ERA-I

Linear Power-law

Mexico techniques compared: profile AA’

School of Earth and Environment

MERIS accuracy

(Z. Li et al., 2006)

Mexico quantification

School of Earth and Environment

• Fixing a reference at the ‘relative’ top of the troposphere allows us to deal with spatially-varying tropospheric delays.

• Band filtering can be used to separate tectonic and tropospheric components of the delay in a single interferogram

• A simple power-law relationship does a reasonable job of modelling the topographically-correlated part of the tropospheric delay.

• Results compare well with weather models, GPS and spectrometer correction methods.

• Unlike a linear correction, it is capable of capturing long-wavelength spatial variation of the troposphere.

Summary/Conclusions

Toolbox with presented techniques will be made available to the community