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Python Source Code - 8.7 KB - MD5: ea6469980355252e0bd5102b24ff2ff2
Dedalus code to compute the eigenfunctions of various solar inertial modes using the Boussinesq setup.
Python Source Code - 5.6 KB - MD5: 3de7d720bebcf37d2f1b875a47e19681
Dedalus code to compute the spectra of modes of the sun in the inertial frequency range, using the Boussinesq setup.
Python Source Code - 9.4 KB - MD5: 0340870ce72e12c3e6c4a6a25804bb78
Dedalus code to compute the eigenfunctions of various solar inertial modes using the compressible setup.
Python Source Code - 5.9 KB - MD5: 976ceeb8f24bcaae9846d7febb79ab2a
Dedalus code to compute the spectra of modes of the sun in the inertial frequency range, using the compressible setup.
Unknown - 458.7 KB - MD5: 3ad302f22396fa39ff66d692005c087b
Data file containing the solar differential rotation profile from Larson & Schou, Sol Phy. 2018, and its corresponding latitudinal entropy gradient.
Unknown - 6.6 KB - MD5: 329d4495181b3a6ef5cbb1b01fbffefa
Details of the conda environment used for the computations.
Plain Text - 1.1 KB - MD5: aa10d9a81efb6fadfe24d53e5e9612a9
README file explaining the details of various files in the directory.
Plain Text - 5.0 KB - MD5: 86d38658793c8d97f40ec7c71879be26
Python dependencies generated from pip.
Unknown - 1.4 MB - MD5: 9ead10c3962ca53c087c0bcc62627ab8
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.
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