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The impact of lateral variations in lithospheric thickness on glacial isostatic adjustment in West Antarctica

Nield, Grace A., Whitehouse, Pippa L., van der Wal, Wouter, Blank, Bas, O'Donnell, John Paul, and Stuart, Graham W., 2018. The impact of lateral variations in lithospheric thickness on glacial isostatic adjustment in West Antarctica. Geophysical Journal International, 214(2):811–824, doi:10.1093/gji/ggy158.

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@ARTICLE{2018GeoJI.214..811N,
       author = {{Nield}, Grace A. and {Whitehouse}, Pippa L. and {van{\^A} der{\^A} Wal}, Wouter and {Blank}, Bas and {O'Donnell}, John Paul and {Stuart}, Graham W.},
        title = "{The impact of lateral variations in lithospheric thickness on glacial isostatic adjustment in West Antarctica}",
      journal = {Geophysical Journal International},
     keywords = {Creep and deformation, Satellite geodesy, Antarctica, Dynamics of lithosphere and mantle, Rheology: crust and lithosphere, Rheology: mantle},
         year = 2018,
        month = aug,
       volume = {214},
       number = {2},
        pages = {811-824},
     abstract = "{Differences in predictions of Glacial Isostatic Adjustment (GIA) for
        Antarctica persist due to uncertainties in deglacial history and
        Earth rheology. The Earth models adopted in many GIA studies are
        defined by parameters that vary in the radial direction only and
        represent a global average Earth structure (referred to as 1-D
        Earth models). Oversimplifying the actual Earth structure leads
        to bias in model predictions in regions where Earth parameters
        differ significantly from the global average, such as West
        Antarctica. We investigate the impact of lateral variations in
        lithospheric thickness on GIA in Antarctica by carrying out two
        experiments that use different rheological approaches to define
        3-D Earth models that include spatial variations in lithospheric
        thickness. The first experiment defines an elastic lithosphere
        with spatial variations in thickness inferred from seismic
        studies. We compare the results from this 3-D model with results
        derived from a 1-D Earth model that has a uniform lithospheric
        thickness defined as the average of the 3-D lithospheric
        thickness. Irrespective of the deglacial history and
        sublithospheric mantle viscosity, we find higher gradients of
        present-day uplift rates (i.e. higher amplitude and shorter
        wavelength) in West Antarctica when using the 3-D models, due to
        the thinner-than-1-D-average lithosphere prevalent in this
        region. The second experiment uses seismically inferred
        temperature as an input to a power-law rheology, thereby
        allowing the lithosphere to have a viscosity structure.
        Modelling the lithosphere with a power-law rheology results in a
        behaviour that is equivalent to a thinner lithosphere model, and
        it leads to higher amplitude and shorter wavelength deformation
        compared with the first experiment. We conclude that neglecting
        spatial variations in lithospheric thickness in GIA models will
        result in predictions of peak uplift and subsidence that are
        biased low in West Antarctica. This has important implications
        for ice-sheet modelling studies as the steeper gradients of
        uplift predicted from the more realistic 3-D model may promote
        stability in marine-grounded regions of West Antarctica.
        Including lateral variations in lithospheric thickness, at least
        to the level of considering West and East Antarctica separately,
        is important for capturing short-wavelength deformation and it
        has the potential to provide a better fit to Global Positioning
        System observations as well as an improved GIA correction for
        the Gravity Recovery and Climate Experiment data.}",
          doi = {10.1093/gji/ggy158},
       adsurl = {https://ui.adsabs.harvard.edu/abs/2018GeoJI.214..811N},
      adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}

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