Abstract
The phenomenon of glacial isostatic adjustment provides uniquely useful information concerning the nature of the planetary mantle. Not only can the observational data be invoked to constrain mantle viscosity but they also provide important clues as to the extent to which the radial profile of mantle density is near adiabatic. Both of these pieces of information are important for the construction of models of the mantle convection process. In this paper I focus on the manner in which the free air gravity anomalies in both Canada and Fennoscandia serve to constrain these two aspects of the radial viscoelastic structure. The results demonstrate the way in which the different horizontal scales of the rebound in these two regions map into differences in the range of depths to which the response is sensitive. A particularly important result concerns the apparent requirement, based upon the free air anomaly over the Canadian Shield, that the seismic horizon at 670 km depth behaves non-adiabatically on the timescale of postglacial rebound.
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© 1989 Kluwer Academic Publishers
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Peltier, W.R. (1989). Glacial Isostasy in Laurentia and Fennoscandia: New Results for the Anomalous Gravitational Field. In: Earthquakes at North-Atlantic Passive Margins: Neotectonics and Postglacial Rebound. NATO ASI Series, vol 266. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-2311-9_7
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DOI: https://doi.org/10.1007/978-94-009-2311-9_7
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