Supplementary figures supporting the corrigendum on the PARASO Geoscientific Model Development paper
- 1. KU Leuven, Belgium
- 2. UCLouvain, Belgium
- 1. UCLouvain, Belgium
- 2. KU Leuven, Belgium
Description
Figures supporting the corrigendum to the PARASO GMD paper. In the original version of the code, the COSMO wind stress were not properly rotated from the COSMO grid to NEMO's. figure_windstress_fix.png provides an illustration of the bug, and the other figures are a selection of diagnostics performed with a fixed version of PARASO, sharing the same experimental design and numbering as the original paper.
Original paper: Pelletier, C., Fichefet, T., Goosse, H., Haubner, K., Helsen, S., Huot, P.-V., Kittel, C., Klein, F., Le clec'h, S., van Lipzig, N. P. M., Marchi, S., Massonnet, F., Mathiot, P., Moravveji, E., Moreno-Chamarro, E., Ortega, P., Pattyn, F., Souverijns, N., Van Achter, G., Vanden Broucke, S., Vanhulle, A., Verfaillie, D., and Zipf, L.: PARASO, a circum-Antarctic fully coupled ice-sheet–ocean–sea-ice–atmosphere–land model involving f.ETISh1.7, NEMO3.6, LIM3.6, COSMO5.0 and CLM4.5, Geosci. Model Dev., 15, 553–594, 10.5194/gmd-15-553-2022, 2022.
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fig_08a.png
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Additional details
Related works
- Is supplement to
- Figure: 10.5281/zenodo.5763819 (DOI)
- Journal article: 10.5194/gmd-15-553-2022 (DOI)