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EXPERIMENTS AT CCRS USING ERS TANDEM MODE DATA
ABSTRACT
1. INTRODUCTIONIn the first experiment we selected a test site on Bathurst Island to evaluate the potential for ERS tandem mission and Radarsat repeat-pass interferometric synthetic aperture radar (InSAR) for DEM generation and scene coherence estimation of Arctic terrain. This is appropriate for repeat-track interferometry because of the desert nature of the terrain (between our data acquisitions there was minimal snow accumulation) and because the low atmospheric water vapour content would minimise propagation inhomogeneities. Successful interferometric pairs were obtained with all the tandem mode data studied and also with RADARSAT 24 day repeat data. As well as the satellite data, high quality airborne cross-track InSAR data was collected using the CCRS CV-580 C-band mapping radar. From this data we have assembled a radar mosaic (~35 x 180 km) of the eastern half of Bathurst data and a digital elevation model with a height noise in the 1 to 3 m rms for most of the radar swath, but increasing to around 4-5 m rms at the swath edge. Height bias errors were minimised by using the sea ice surrounding Bathurst Island. This data is sufficiently accurate to use as a reference data set against which to evaluate the results of the satellite InSAR mapping experiment. In the second experiment, ERS tandem mode image pairs were used to track ice movement of the Saskatchewan Glacier in the Canadian Rockies. This glacier is very accessible and the results of the experiment have been compared with good historical data and with in-situ ice movements obtained by traditional glaciological techniques.
For both test sites precise ERS orbit data generated by GFZ Potsdam (Massmann et al., 1993) and digital elevation models (DEMs) obtained from the CCRS airborne interferometric SAR (InSAR) system were used. The ERS interferometric imaging geometry was reconstructed using the accurate orbit data which, together with the airborne InSAR DEM, allowed the calculation of the expected slant range interferogram from the tandem pair. By forming the product of the predicted interferogram with the complex conjugate of the actual interferogram, the influence of topography can be removed and information related to ground movement, or atmospheric propagation inhomogeneities, is observed in the residual phase. For the Arctic test sites results will be shown for 4 tandem mode pairs and the non-uniformity of the differential phase is explained in terms of residual propagation inhomogeneities. Phase errors in the range of 1 to 2 radians on scales of 1 to 10's of km were observed. These phase errors appear not to be related to errors in the digital terrain model or orbit knowledge and may impact the accuracy of terrain movement estimation and of extracted topography, depending on the baseline. Saskatchewan Glacier movement has been the focus of previous studies (Vachon et al., 1996) in which 5 pairs of ascending pass ERS tandem mode data were used to satisfactorily measure the glacier's flow rate, as validated by in situ point surveying measurements. In this work, we extend the data set to also consider the descending passes in an attempt to obtain a more accurate flow field determination. However, it is now evident that the descending pass geometry is worse (the projection of the motion vector along the radar line of site for the descending passes is small and leads to a less accurate estimate). Even two observations with different geometry's are not adequate to solve for the 3-D flow field. 2. ARCTIC EXPERIMENTA perspective view of our test site on Bathurst island of the Canadian arctic, generated from an accurate digital terrain model (DTM) by CV-580 InSAR system, is shown in Figure 1. The barren, rocky, wind-swept, vegetation free terrain ensured high coherence for the ERS tandem interferometry repeat pass experiment. Four similar tandem pairs, all ascending and all with the same relative orbit (RO) were selected. These are detailed in Table 1. The ERS interferometric processing used is described in detail elsewhere (Geudtner, 1995). Basically, the SLC images were first co-registered using a cross-correlation analysis. The images were then filtered in range and azimuth. The range filtering selects only overlapping portions of the object spectrum based on a spectral analysis of the interferogram to determine the fringe frequency. The azimuth filtering suppresses non-overlapping portions of the azimuth Doppler spectra resulting from processing with different Doppler centroid frequencies. The filtered images were then oversampled by a factor of two in both range and azimuth, and the interferogram was formed. The coherence is then estimated using an averaging window size of 50 (azimuth) by 10 (range) samples and corrected for finite signal-to-noise ratio. Since the azimuth and range filtering avoid decorrelation due to spectral misalignment and the measured coherence has been corrected for finite signal-to-noise ratio, the resulting coherence estimate may be interpreted as the temporal scene coherence. The scene coherence for the four tandem pairs considered here are shown in Figure 2. The scene coherence in all cases is very high except for the dark pattern which correlate well with the drainage network, where isolation from the wind results in snow accumulation or changes in the snow crystalline structure.
Table 1: Summary of ascending passes of ERS-1/2 data over Bathurst Island The interferogram phase is given by:
where
where Bn is the normal component of
the baseline,
where We make use of the digital terrain model (DTM) derived from the CV-580 InSAR system (Mattar et al., 1994,) to remove the topographic component from the interferogram phase. With the use of the precise orbit data, PRC, supplied by D-PAF (Massmann et al., 1993), and using a modification of the algorithm described by Geudtner & Schwäbisch (1996), we project the DTM from UTM co-ordinates into phase in the ERS-1 slant range perspective. We then manually optimise the registration between the ERS interferogram and the synthetic interferogram, in both azimuth and range, by comparing the magnitude images. The differential interferogram is then created by subtracting the two interferogram phase components. Furthermore, a least-square best linear trend in azimuth and range is removed from the differential phase to account for first order residual orbit data inaccuracies and atmospheric heterogeneities. The linear trend removed varied from 0.0 to 0.5 radians over a 10 km scene. The resulting differential interferogram phase shown in Figure 3.
The residual phase shown in Figure 3,
showing at times a wavelike pattern, has a peak to peak amplitude
of approximately 1 radian with RMS values in uniform areas
between 0.13 and 0.25 radians. Even in the case of the largest
tandem baseline, an error of more than 50 m in the DTM would be
necessary to account for this residual phase. This discounts The ever present possibility of substantial atmospheric
component to the interferogram phase has implications for the use
of repeat pass satellite interferometry for both DEM generation
and displacement measurements. In the former case, choosing a
large baseline (under the constraints imposed by scene
decorrelation), enables the minimisation of Unfortunately this flexibility is not available when using interferometry for displacement measurements. Furthermore the unpredictable nature of these effects makes it difficult to subtract them out with use of control points. The effect can be reduced by averaging a number of independent measurements, or when measuring displacements that are large with respect to nominal atmospheric effects. 3. GLACIER EXPERIMENT The Saskatchewan glacier was the focus of a previous study where 5 ascending ERS tandem passes were used to estimate the flow field of the glacier (Vachon et al., 1996). We now expand the study, and seek to improve the estimate of the flow field by using both ascending and descending ERS tandem passes. The same procedure listed above is used to generate the interferogram and scene coherence. A representative tandem mode interferogram from November 2/3, 1995 is shown in Figure 4. The top two panels represent the interferogram magnitude and scene coherence. The lower panels represent the raw and flat-earth corrected phase, in both cases wrapped in intervals of 2. From the top we see Dome, Athabasca, and Saskatchewan glaciers. Among all the ERS tandem passes available only five ascending passes and four descending passes had sufficient coherence over the Saskatchewan glacier to be of use. These are listed in Tables 2 and 3 respectively.
Table 2: Summary of coherent ERS-1/2 ascending passes over Saskatchewan glacier
Table 3: Summary of coherent ERS-1/2 descending passes over Saskatchewan glacier The differential interferogram is created as described in the previous section using an accurate DEM obtained from the CV-580 InSAR system ( Figure 5) and PRC data from D-PAF. The differential interferograms were unwrapped, converted to line-of-sight displacement (LOS) using equation (3), and mapped back to UTM co-ordinates. Figure 6 and 7 show the LOS displacement R along the centrelines of the glacier for the ascending and descending Tandem passes respectively. Unlike the differential interferograms in the previous section, the difficult terrain in this case did not permit the removal of the best linear fit from this data set.
There may, therefore, be a linear trend in azimuth and/or in range. Without any other means of monitoring the atmosphere, there may be an atmospheric phase component as well. From the previous section, the linear trend could amount to up to 0.5 radians or 0.25 cm LOS over the scene, and the atmospheric phase component could be on the order of a radian, or 0.5 cm LOS. We cannot, therefore, rule out the possibility that the differences observed in the various ascending and descending LOS displacements in Figures 6 and 7 could be due to linear offset or atmospheric effects rather than real differences in the LOS displacement on the various dates. Nevertheless, these differences are small compared to the overall displacement observed.
For the calculation of the surface displacement field we choose to use the March 5/6 LOS displacement from the ascending pass and the March 10/11 LOS displacement for the descending pass. They are closely spaced in time. They also have an average trend compared to the other ascending and descending passes. The surface displacement field is measured by the repeat pass interferometry as projected along the radar LOS R. The surface displacement is given as (Vachon et al., 1996):
The geometry is shown in Figure 8. u is the angle between the vertical and local surface normal (varying between 0o and 180o), and v is the angle between x axis and the projection of the local surface normal on to the horizontal (varying between 0o and 90o).
Equation (4) has three unknowns: D, u and v. Since we have available both the ascending and descending LOS displacements, we can use equation (4) twice. We still need an assumption to solve for the displacement D. At least three different assumptions can be considered: (1) if the glacier flows in the direction of greatest slope, v can be calculated from the DEM. (2) v can be calculated assuming the flow is in the direction of the glacier centreline. (3) assuming the glacier flows parallel to the glacier surface zt(x,y), then the vertical velocity is related to the horizontal velocity by (Joughin et al., 1996):
Equation (5) can then be used in combination with equation (4) to solve the D. Figure 9 is a plot of the displacement derived using each of these three assumptions. Also included in Figure 9 are historic and recent glacier flow measurements obtained the traditional (and very time consuming) triangulation method. Each of the assumptions have their disadvantage. Assumption (1) obviously fails near the 4500 mark. This coincides with the area near the bend in the glacier where glacier v reaches nearly 70o. The glacier is moving in the direction of the glacier centreline rather than in the direction of greatest downslope gradient. Assumption (3) applies only in portions of the glacier at steady state. It fails in regions of accumulation or ablation, where the flow is no longer parallel to the surface (Joughin et al., 1996). Nevertheless, it appears to be the best assumption of the three. 4. CONCLUSIONThe Bathurst Island ERS tandem mode data shows that even in Arctic terrain under winter conditions there are atmospheric conditions which will affect radar wave propagation. The resulting interferogram differential phase from the combination of a pair of passes will have fluctuations of magnitude 1 to 2 radians due to these propagation anisotropies.. With a small baseline, as was obtained with the tandem mode data, this means that topographic information can be in error by many tens of metres. However, if the baseline is much larger (as has been obtained with RADARSAT fine mode data pairs) and with use of ground control points to create fictive satellite positions, the error from this source can be reduced to less than 10 meters. In the Saskatchewan Glacier movement experiment the combination of data from both ascending and descending passes has helped address the problem of which assumption to make in converting a line-of-sight displacement to a glacier flow field. 5. ACKNOWLEDGEMENTSESA provided the ERS SAR data and D-PAF (GFZ Potsdam) provided the ERS orbit data. We thank M. Brugman (Columbia Mountains Institute of Applied Ecology), I. Cumming (UBC/EE), and J.-L. Valero (UBC/EE) for their contribution to the Saskatchewan Glacier study. G.D.'s contribution to this work was supported by an ESA fellowship. 6. REFERENCES
[1] Under contract from Intermap at CCRS. [2] Now working at DLR, Institute of Radio Frequency Technology. Keywords: ESA European Space Agency - Agence spatiale europeenne, observation de la terre, earth observation, satellite remote sensing, teledetection, geophysique, altimetrie, radar, chimique atmospherique, geophysics, altimetry, radar, atmospheric chemistry |
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