Routines and notebooks for computing iceberg trajectories and melting offline
- so far supports reading (interpolated) forcing data from the COSMOS climate model and AWI-CM
- code is based on the Fortran code of FESOM-IB
The Fortran source can be found here, after registration at swrepo1.awi.de.
The analysis for the submitted paper
'An Antarctic Iceberg Melt Driver of Glacial Deep Water-Mass Reorganizations' by Aidan Starr, Ian R. Hall, Stephen Barker, Thomas Rackow, Xu Zhang, Sidney R. Hemming, H.J.L van der Lubbe, Gregor Knorr, Melissa A. Berke, Grant R. Bigg, Alejandra Cartagena, Francisco J. Jiménez-Espejo, Xun Gong, Jens Gruetzner, Nambiyathodi Lathika, Leah J. LeVay, Rebecca S. Robinson, Martin Ziegler, and the Exp. 361 Science Party
can be reproduced with the following Jupyter notebook.
Southern Ocean Iceberg Melt under pre-industrial (PI) vs last glacial maximum (LGM) conditions
(left) Iceberg trajectories, (middle) sea surface temperature, and (right) iceberg probability between 0-50°E in the Southern Ocean under PI and LGM conditions, using pyberg forced with COSMOS climate model output.