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Polar Marine Gravity fields from ERS-1
Abstract
IntroductionGeophysical survey in the polar regions has long been hampered by the inaccessibility of the polar regions, particularly in areas which suffer permanent coverage by sea ice. In some areas of the polar oceans less is known about the ocean floor than is known about the surface of Mars or the Moon. As a result some of the last remaining uncertainties in global tectonic models lies in the tectonic evolution of the Arctic Ocean and the seas surrounding Antarctica.In fact, major, missing tectonic plate boundaries, presumably active during the Cretaceous and/or early Tertiary, have been hypothesised for both the Arctic(Vogt, et. al., 1979) and Antarctic(Stock and Molnar, 1987)(Cande, et. al., 1995). Proof that these plate boundaries actually existed and the actual delineation of their specific location has not been possible due to the acute sparsness of surface surveys. High-resolution marine gravity fields derived from ERS-1 altimeter data are now providing the answer to these long standing problems in the tectonic evolution of the polar regions. Altimetry Over Sea IceHigh precision satellite altimeter measurements of sea surface topography are achieved by emitting a short (3ns) pulse and measuring the delay time to receipt of a return echo from the surface. To achieve this a spaceborne altimeter must predict the delay time at which the next echo is to be received. This is necessary because the distance over which the echo recorded is much shorter than the total variations of distance from the satellite to the ground, due to the orbit being non-circular and due to variations in the Earth's topography. This is achieved by using a 'tracker' on board the satellite which analyses the previous echo to estimate the arrival time of the next. These onboard estimates of the range to the surface are included in the telemetry and over open ocean are used to determine the surface elevation. Over sea ice, however, the onboard estimates suffer noise because the tracker is not designed to cope with the specular returns which occur over sea ice.
Figure 1(a)shows a sequence of return echoes from the open ocean whilst figure 1(b) shows a sequence over an area covered by sea ice. The vertical dashed lines shown in figure 1 correspond to position of the leading edge of the return echo waveform determined by the tracker onboard ERS-1. For returns from the open ocean the onboard processor correctly identifies the location of the leading edge of the return echo, corresponding to a return from the sub-satellite point. Over sea ice, however, the position of the leading edge determined by the onboard processor is in error by several metres. The origin of these errors lies in the fact that the on-board processor assumes a model for the return echo based on reflection from open water. This effect can be seen in Figure 2(a) where a dramatic increase in height noise accompanies the transition from open ocean to sea ice. The small variations in sea surface height, associated with tectonic features, are completely obscured. To reduce this noise it is necessary to reprocess the altimeter echoes recorded by the spacecraft. To achieve this requires the use of the full echo waveform (WAP) data rather than the ocean product (OPR) data set, normally used for open ocean gravity mapping, which contains only on-board estimates of surface height. By measuring the offset between the range to leading edge of the recorded echo and the range estimated by the on-board processor a correction can be computed(Laxon, 1994). By applying this correction to the on-board estimates the height noise is significantly reduced. Figure 2(b) shows the same height profile as Figure 2(a) but corrected for tracking errors. As can be seen the noise associated with tracker error has been significantly reduced. By selecting data in areas of seasonal sea ice the corrected profile can be compared with data obtained at a different time when no ice is present. The profile in figure 2(c) covers the same ground track as the data shown in figure 2(a) and figure 2(b) but was acquired when no ice was present. Such data can be used to assess how well the retracking algorithm is working when ice is present. After the removal of outliers and the elimination of some spurious signals due to the ice cover individual height profiles are smoothed and then differentiated to extract along-track slopes. Grids of ascending and descending slopes are then generated and gravity anomalies calculated using the method of McAdoo and Marks(McAdoo and Marks, 1992).
ERS Marine Gravity Over Sea IceThe ERS-1 satellite, launched in July 1991, provided coverage of the polar oceans up to 82 degrees for the first time. A large fraction of the new areas surveyed are covered by seasonal or permanent areas of sea ice. However, following the launch of ERS-1, a study of the altimeter tracking performance revealed that the altimeter frequently lost lock of the leading edge of the return echo over sea ice(Scott, et. al., 1994). This problem seriously affected data acquired in ocean mode and to a lesser extent that acquired in ice mode. The ice mode of ERS-1 was designed specifically to cope with rapid variations in surface topography occurring over the large terrestrial ice sheets. Whilst ice mode was not specifically designed for operation over sea ice, it did afford better tracking over sea ice areas, albeit with a poorer resolution of surface height measurements due to the wider bin width.An error in ground command programming lead to the operation of ERS-1 in ice mode over most of the Arctic Ocean for several 35 day repeat cycles starting in June 1992 (Cycle 86). The processing of an incomplete data set from this cycle of ERS-1 lead to the first marine gravity field over the Arctic Ocean including permanently ice covered areas. Although the resolution of this field was only 70 km, it provided the first satellite altimeter derived marine gravity field over the Arctic Ocean and lead to significant geophysical discoveries (Laxon and McAdoo, 1994). ESA continued, with assistance from MSSL, to try and rectify the problems in tracking over sea ice areas. After a number of software patches continuous tracking over sea ice was finally achieved in June 1993. Cycles 96 and 97 which followed provided the first complete coverage in Ocean mode and allowed the generation of an improved gravity field based on three cycles of data. In April 1994 ERS-1 started it's geodetic mission from which the current fields are generated. In addition ERS data from the tandem mission was added in selected areas, in particular in the Bellingshausen Sea, where we suspected the tectonically important signatures of fracture zones might be discovered.
ResultsFigure 3 shows the marine gravity map for the Arctic Ocean for all areas up to 82N. The new gravity data reveal a wealth of detail on the structure of the Arctic ocean floor. The gravity field clearly shows the margin of the deep Arctic Basin. The Chukchi Borderland is revealed as a complex system of gravity highs and lows perhaps representing stretched continental crust. The southern tip of the Mendeleev ridge is also seen although it's gravitational signal is somewhat enigmatic. The Eastern margins of the Lomosonov and Nansen ridges lying in the deep Arctic basin also appear clearly in our gravity field. Over the broad Eurasian continental shelf numerous geological structures are observed the nature of which is still the subject of investigation. The a most significant discovery in the Arctic is linear gravity low trending roughly North-South in the Canada Basin. This lineation is now believed to represent the signature of the extinct spreading ridge, lying beneath several km of sediment, which was responsible for the opening of the Canada basin some 100 million years ago(Laxon and McAdoo, 1994). Figure 4 shows the new gravity field of the Southern Ocean. ERS-1 marine gravity has been used for all areas from 160E east to 0W. In other areas data from the Geosat geodetic mission are shown (McAdoo and Marks, 1992). Although the new areas revealed in our gravity data are smaller than in the Arctic, the results are highly significant from a tectonic point of view. Much of the Weddell sea is previously unmapped and a number of tectonically significant features are observed(McAdoo and Laxon, 1996). The poorly mapped continental margin of the West Antarctic is clearly observed in our gravity field. Perhaps the most significant result are the faint N-S trending gravity lineations on the Pacific margin of Antarctica (200 - 220E). These correspond to the fracture zones created by the separation of the Campbell Plateau from Antarctica some 80 million years ago. By matching the fracture zone traces adjacent to Antarctica with conjugate traces near the Campbell Plateau we have reconstructed the relative positions of the two continents some 67 million years ago. The reconstruction reveals an offset in the fracture zones further east which we attribute to the existence of the previously hypothesised Bellingshausen plate(McAdoo and Laxon, 1997). ValidationFigure 5 shows a comparison between the ERS-1 marine gravity with that obtained from an aircraft survey carried out by the Naval Research Lab. Agreement between the longer wavelength components is extremely close. At shorter wavelengths the ERS-1 gravity reveal oscillations which are likely caused by height errors left by retracking over sea ice. We estimated the resolution of the original Arctic Ocean gravity as around 70km. Figure 6 shows a coherence plot of the ERS-1 and NRL airborne survey data.This analysis shows that the two data types agree to wavelengths as short as 30-40km where coherency falls below 0.5. The limiting factor in the current fields appears to be the remaining noise on the retracked heights obtained over sea ice.
ConclusionsERS-1 has provided the first view of some of the most poorly mapped areas of the ocean floor. The results have solved two major remaining problems in the Earth's tectonic history, namely the origin of the Canada Basin and the existence of the Bellingshausen plate. Our efforts are now concentrated on better understanding the nature of the height signal obtained over sea ice in terms of the instrument response to the return echoes. Forthcoming data from ERS-2 will be added to our fields to significant reduce the remaining noise in height retrievals allowing further refinement of our fields. In the meantime to permit the full exploitation of this data by the geophysical community we will be releasing some of our gravity fields on the WWW.AcknowledgementWe acknowledge ESA for supplying the WAP product, Richard Francis for his efforts in fixing the altimeter tracking and Skip Kovacs, John Brozena, Mary Peters and Vicki Childers of the Naval Research Lab for the Airbone gravity.
References
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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