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Large scale studies on ice shelves
      ERS-1/2 1992-2001        ERS-2/Envisat 1994-2008         ICESat 2003-2008




         Zwally et al., 2005        Shepherd et al., 2010       Pritchard et al., 2012


    Duration   9 years               14 years                       5 years
    Spat. Res. 100 km                One value per ice shelf        30 km
    Time Res. 3 months               35 days (!)                    1-2 years

    This study: ERS-1/ERS-2/Envisat 1992-2012                                            2

*
The need for multi-mission RA

          Long vs short records in detecting climate trends

                                            How long?
                                            Decadal records
                                            (20+ years)

                                            Interannual and
                                            decadal variability
                                            unexplored
                                           Fricker and Padman, 2012



    Our goal → to capture the variability in space and time on the
    ice shelf spatial scales: 20+ years / 20-30 km                3

*
Penetration depth (backscatter)

                           Penetration depth:

                           ! Water ! "(mm)
                           ! Wet snow ! O(cm)

                           ! Dry snow ! O(m)



                           !   And varies with time
                      A




                                     Radar
                                     penetrates
                                     into firn layer

                      B
                                                       4

*
Constructing time series of dh

                 Similar (but not the same) method as
    Davis & Segura (2001), Zwally et al. (2005), Khvorostovsky (2011).




                                                                         5

*
Averaging in time and space
    1 vs 3-month averages
                            less crossovers
                            per bin → larger
                            error bars
                            improved signal-to-
                            noise ratio and no
                            gaps


                                  20-30 km bins




                                                  6

*
Crossing all possible time combinations

     Now we have one time series per reference time: t1, t2, t3, ...




     These are elevation changes with respect to different epochs


                                                                       7

*
One grid per time combination

    Crossovers   t1
                                ~ 1500 grids
                      t2
                           t3




                                               8

*
Multi-referenced time series
    At every individual grid-cell we have now several time series




                                                         outliers




     1) To align we use average of the offset for overlap period only

     2) Then we frequency-weighted average the aligned time series      9

*
Cross-calibration of average TS
    Cross-calibration is done using overlap periods between missions
      dh = elevation change           dAGC = backscatter power change




               ERS-1          ERS-2             Envisat




                                                                        10

*
Backscatter correction (approach 1)
                        By correlating absolute values ! dAGC x dh




                                                                     11
Wingham et al., 1998; Davis & Ferguson, 2004; Zwally et al., 2005
Backscatter correction (approach 1)
    By correlating absolute values ! dAGC x dh
Backscatter correction (approach 2)
   By correlating differences ! diff(dAGC) x diff(dh)
Backscatter correction (approach 3)
    By time variable correlation ! R(t) and S(t)




                                                   14
Backscatter correction (approach 3)
    By time variable correlation ! R(t) and S(t)




                                     Correlation

                                      Sensitivity




                                                    15
Correlation and Sensitivity maps
      FRIS



(1)




(2)




                                                16
Correlation and Sensitivity maps



(1)


      ROSS




(2)




                                          17
Now some results




                   18
High spatial and temporal variability




20-year trend in elevation change
(original grid)

                                                 19
High spatial and temporal variability




20-year trend in elevation change
(original grid)

                                                                                        20
                                    Obs: 2001 was chosen to avoid a big calving event
20-year trend in
elevation change
(original grid)




Obs: 2001
was
chosen to
avoid a
big calving
event              21
High interannual variability




                               22
Coherent changes?
Tracking coherent events around the Antarctic margin
How well do we know what RA is measuring?




                                                24

*
Envisat vs ICESat

                        We follow
                        the ICESat
                        campaigns




                                 25

*
Envisat vs ICESat




*
Conclusions
!
    Multi-mission RA can be used to construct continuous
    long records with their variability content
!
    There is a lot of variability both in time and space
!
    Variability is the key to understand forcings and climate-
    induced changes (ocean and atmospheric circulation)
!
    Relative error (precision) vs absolute error (penetration)
!
    Different b/s approaches yield different results?
!
    How can we validate b/s correction when there are so little
    ground truthing data and in practice:


                                                                 27
We thanks
!
    NASA NESSF Fellowship
!
    Jay Zwally & Jairo Santana (NASA/GSFC)
!
    Curt Davis (UM) & Duncan Wingham (UCL)
!
    NASA grants NNX06AD40G and NNX10AG19G
!
    ESA for ERS-1, ERS-2 and Envisat altimeters!
!
    San Diego Super Computer Center
!
    Geir Moholdt
!
    Python and Open Source



                                                   fpaolo@ucsd.edu

                                                                     28
Antarctic ice shelf mask

    A reliable and complete ice shelf mask is a problem
    So we (Geir Moholdt) created our own using all data available: MOA (Scambos
    et al. 2007), ASAID (Bindschadler et al. 2011), InSAR (Rignot et al. 2011),
    ICESat (Fricker/Brunt et al. 2006-10)




                                                                              29

*
Backup slide




               30
Challenges of multi-mission integration
!
    Differences between missions:
    - RA systems, orbit configurations, time spans...
!
    Radar interaction with time variable surface properties
!
    Spatial and temporal dependent corrections:
    - Ocean tides (for high lat)
    - Atm pressure (IBE)
    - Surface density (firn densification)
    - Penetration depth (backscatter)


                                                          31
How to reduce the noise?


    !
        Due to hydrostatic equilibrium the altimeter only see 10%
        of the grounded ice signal (in elevation change)


    !
        So to increase signal-to-noise ratio → requires lots of
        averaging both in time and space




                                                                    32

*
The uncertainty
!
    How well do we know the error?
!
    What do error bars in the time series actually represent?




    After all the averaging a mean error is: ± 5-20 cm over 20-30 km


!
    What about the uncertainty in penetration depth?
    O(m/cm)


                                                                       33

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Interannual and decadal variability of Antarctic ice shelf elevations from multi-mission satellite radar altimetry

  • 1.
  • 2. Large scale studies on ice shelves ERS-1/2 1992-2001 ERS-2/Envisat 1994-2008 ICESat 2003-2008 Zwally et al., 2005 Shepherd et al., 2010 Pritchard et al., 2012 Duration 9 years 14 years 5 years Spat. Res. 100 km One value per ice shelf 30 km Time Res. 3 months 35 days (!) 1-2 years This study: ERS-1/ERS-2/Envisat 1992-2012 2 *
  • 3. The need for multi-mission RA Long vs short records in detecting climate trends How long? Decadal records (20+ years) Interannual and decadal variability unexplored Fricker and Padman, 2012 Our goal → to capture the variability in space and time on the ice shelf spatial scales: 20+ years / 20-30 km 3 *
  • 4. Penetration depth (backscatter) Penetration depth: ! Water ! "(mm) ! Wet snow ! O(cm) ! Dry snow ! O(m) ! And varies with time A Radar penetrates into firn layer B 4 *
  • 5. Constructing time series of dh Similar (but not the same) method as Davis & Segura (2001), Zwally et al. (2005), Khvorostovsky (2011). 5 *
  • 6. Averaging in time and space 1 vs 3-month averages less crossovers per bin → larger error bars improved signal-to- noise ratio and no gaps 20-30 km bins 6 *
  • 7. Crossing all possible time combinations Now we have one time series per reference time: t1, t2, t3, ... These are elevation changes with respect to different epochs 7 *
  • 8. One grid per time combination Crossovers t1 ~ 1500 grids t2 t3 8 *
  • 9. Multi-referenced time series At every individual grid-cell we have now several time series outliers 1) To align we use average of the offset for overlap period only 2) Then we frequency-weighted average the aligned time series 9 *
  • 10. Cross-calibration of average TS Cross-calibration is done using overlap periods between missions dh = elevation change dAGC = backscatter power change ERS-1 ERS-2 Envisat 10 *
  • 11. Backscatter correction (approach 1) By correlating absolute values ! dAGC x dh 11 Wingham et al., 1998; Davis & Ferguson, 2004; Zwally et al., 2005
  • 12. Backscatter correction (approach 1) By correlating absolute values ! dAGC x dh
  • 13. Backscatter correction (approach 2) By correlating differences ! diff(dAGC) x diff(dh)
  • 14. Backscatter correction (approach 3) By time variable correlation ! R(t) and S(t) 14
  • 15. Backscatter correction (approach 3) By time variable correlation ! R(t) and S(t) Correlation Sensitivity 15
  • 16. Correlation and Sensitivity maps FRIS (1) (2) 16
  • 17. Correlation and Sensitivity maps (1) ROSS (2) 17
  • 19. High spatial and temporal variability 20-year trend in elevation change (original grid) 19
  • 20. High spatial and temporal variability 20-year trend in elevation change (original grid) 20 Obs: 2001 was chosen to avoid a big calving event
  • 21. 20-year trend in elevation change (original grid) Obs: 2001 was chosen to avoid a big calving event 21
  • 23. Coherent changes? Tracking coherent events around the Antarctic margin
  • 24. How well do we know what RA is measuring? 24 *
  • 25. Envisat vs ICESat We follow the ICESat campaigns 25 *
  • 27. Conclusions ! Multi-mission RA can be used to construct continuous long records with their variability content ! There is a lot of variability both in time and space ! Variability is the key to understand forcings and climate- induced changes (ocean and atmospheric circulation) ! Relative error (precision) vs absolute error (penetration) ! Different b/s approaches yield different results? ! How can we validate b/s correction when there are so little ground truthing data and in practice: 27
  • 28. We thanks ! NASA NESSF Fellowship ! Jay Zwally & Jairo Santana (NASA/GSFC) ! Curt Davis (UM) & Duncan Wingham (UCL) ! NASA grants NNX06AD40G and NNX10AG19G ! ESA for ERS-1, ERS-2 and Envisat altimeters! ! San Diego Super Computer Center ! Geir Moholdt ! Python and Open Source fpaolo@ucsd.edu 28
  • 29. Antarctic ice shelf mask A reliable and complete ice shelf mask is a problem So we (Geir Moholdt) created our own using all data available: MOA (Scambos et al. 2007), ASAID (Bindschadler et al. 2011), InSAR (Rignot et al. 2011), ICESat (Fricker/Brunt et al. 2006-10) 29 *
  • 31. Challenges of multi-mission integration ! Differences between missions: - RA systems, orbit configurations, time spans... ! Radar interaction with time variable surface properties ! Spatial and temporal dependent corrections: - Ocean tides (for high lat) - Atm pressure (IBE) - Surface density (firn densification) - Penetration depth (backscatter) 31
  • 32. How to reduce the noise? ! Due to hydrostatic equilibrium the altimeter only see 10% of the grounded ice signal (in elevation change) ! So to increase signal-to-noise ratio → requires lots of averaging both in time and space 32 *
  • 33. The uncertainty ! How well do we know the error? ! What do error bars in the time series actually represent? After all the averaging a mean error is: ± 5-20 cm over 20-30 km ! What about the uncertainty in penetration depth? O(m/cm) 33