GSTM2022-32
https://doi.org/10.5194/gstm2022-32
GRACE/GRACE-FO Science Team Meeting 2022
© Author(s) 2022. This work is distributed under
the Creative Commons Attribution 4.0 License.

150 km ANU mascon solutions

Paul Tregoning1, Rebecca McGirr1, Anthony Purcell1, and Sebastien Allgeyer2
Paul Tregoning et al.
  • 1The Australian National University, Research School of Earth Sciences, Earth Physics, CANBERRA, Australia (paul.tregoning@anu.edu.au)
  • 2Geoscience Australia, Symondston, CANBERRA, Australia

We present updated mascon solutions of the temporal gravity field, derived from the analysis of Level-1B GRACE and GRACE-FO data using the range acceleration observable. Our previous solutions contained significant noise in particular regions of high mass loss (e.g. West Antarctica), which was caused by inappropriate levels of regularisation. Here we show a new approach of both iteration and regularisation of the solutions which generates more reliable estimates of the mass variations across the whole Earth, with both temporal and spatial consistency despite not applying any temporal or spatial inter-mascon constraints. We compare mascon solutions at spatial resolutions from 300 km to 100 km, show estimates of ocean mass increase and mass loss in ice-covered regions as well as assess the C20 time series estimated directly from GRACE data alone. Our new mascon estimates, at ~200 km x 200 km spatial resolution, are now publicly available.

How to cite: Tregoning, P., McGirr, R., Purcell, A., and Allgeyer, S.: 150 km ANU mascon solutions, GRACE/GRACE-FO Science Team Meeting 2022, Potsdam, Germany, 18–20 Oct 2022, GSTM2022-32, https://doi.org/10.5194/gstm2022-32, 2022.

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