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Plain Text - 5.0 KB - MD5: 86d38658793c8d97f40ec7c71879be26
Python dependencies generated from pip.
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Data file for the n = 0 equatorial Rossby mode with azimuthal order m = 3, obtained from the compressible setup
Jupyter Notebook - 2.9 MB - MD5: d5d251ff0bdb1fa25fe38843442e7c6c
Sample Jupyter notebook for plotting the eigenfunctions of the solar inertial modes. It plots the eigenfunction of the n = 0 equatorial Rossby mode with azimuthal order m = 3, computed using the compressible setup. It can be modified to plot the eigenfunctions of the other computed inertial modes.
TAR Archive - 20.4 GB - MD5: 48197d4472cbffdfc5bfd4c2c3b264dc
Only the parameters of SMPLH +D and object for all frames
ZIP Archive - 5.3 GB - MD5: 4820042084bb643f930120c7ef857cec
SampleDatasets and Annotations for 3D-SOCS
Plain Text - 13.0 GB - MD5: 29ae52c080f760c1e7e13a2ec876d57b
DATA
Plain Text - 2.4 GB - MD5: 7ad20451cb42d178b309b11786aebfca
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