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doreenfan
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This PR includes a set of subroutines in /Util/postprocess/ to compute various diagnostics for the fully convective star problem by post-processing amrex-generated plot files.

A valid plot file will need to be provided as an input parameter. If such a file is not provided, the code will generate a sample (exact solution) plot file that can be used to verify the code. Please refer to the README file for more details on additional input parameters.

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ajnonaka commented Aug 24, 2020

The updated notes from Adam:
measures.pdf

ajnonaka and others added 30 commits September 14, 2020 07:24
…initial data before summing integrated quantities over time
…_solver and maestro.hg_bottom_solver

default is on (4) for both mg and hg
set it to any other value to use the default MLMG settings
…ing O(1) differences in runs depending on the number of MPI processors. This change may need to be put into development ahead of merging this branch.
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4 participants