-
-
Notifications
You must be signed in to change notification settings - Fork 16
Commit
This commit does not belong to any branch on this repository, and may belong to a fork outside of the repository.
- Loading branch information
1 parent
a5343d9
commit 3de3604
Showing
8 changed files
with
1,482 additions
and
0 deletions.
There are no files selected for viewing
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -0,0 +1,50 @@ | ||
{ | ||
"cells": [ | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [ | ||
"# Using a MESA model" | ||
] | ||
}, | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [ | ||
"Using a MESA model entails a few changes in the utilization of STARDIS. Firstly, you must change the model type to 'mesa' under the 'model' section, like this: \n", | ||
"\n", | ||
"```\n", | ||
"model:\n", | ||
" type: mesa\n", | ||
" fname: end_core_h_burn.mod\n", | ||
"```\n" | ||
] | ||
}, | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [ | ||
"Next, you can now specify the outmost depth point for the simulation using the 'truncate_to_shell' parameter. It defaults to -99, which tells the model to use all shells. Place the parameter in the 'model' section, like this: \n", | ||
"```\n", | ||
"model:\n", | ||
" type: mesa\n", | ||
" fname: end_core_h_burn.mod\n", | ||
" truncate_to_shell: 40\n", | ||
"```" | ||
] | ||
}, | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [] | ||
} | ||
], | ||
"metadata": { | ||
"language_info": { | ||
"name": "python" | ||
}, | ||
"orig_nbformat": 4 | ||
}, | ||
"nbformat": 4, | ||
"nbformat_minor": 2 | ||
} |
This file contains bidirectional Unicode text that may be interpreted or compiled differently than what appears below. To review, open the file in an editor that reveals hidden Unicode characters.
Learn more about bidirectional Unicode characters
Original file line number | Diff line number | Diff line change |
---|---|---|
@@ -0,0 +1,114 @@ | ||
{ | ||
"cells": [ | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [ | ||
"# Running the Simulation in Parallel" | ||
] | ||
}, | ||
{ | ||
"cell_type": "markdown", | ||
"metadata": {}, | ||
"source": [ | ||
"You can change the number of threads that STARDIS uses with the n_threads keyword. \n", | ||
"A few things to remember when running STARDIS in parallel: \n", | ||
" \n", | ||
"If no n_threads argument is provided, it defaults to 1 and runs in series. \n", | ||
" \n", | ||
"Set n_threads to 0 to use all available threads. \n", | ||
" \n", | ||
"The n_threads argument must be between the config version and the atom data, like this: \n", | ||
"```\n", | ||
"stardis_config_version: 1.0 \n", | ||
"n_threads: 4 \n", | ||
"atom_data: kurucz_cd23_chianti_H_He.h5\n", | ||
"```\n", | ||
"\n", | ||
"In the [stardis_config_parallel](stardis_config_parallel.yml) file, an n_threads value of 4 is added to the example config. Try running this code yourself to see how n_threads affects STARDIS's efficiency." | ||
] | ||
}, | ||
{ | ||
"cell_type": "code", | ||
"execution_count": 1, | ||
"metadata": {}, | ||
"outputs": [ | ||
{ | ||
"data": { | ||
"application/vnd.jupyter.widget-view+json": { | ||
"model_id": "25723fa78e8d43ef8129a7667a39ebf8", | ||
"version_major": 2, | ||
"version_minor": 0 | ||
}, | ||
"text/plain": [ | ||
"Iterations: 0/? [00:00<?, ?it/s]" | ||
] | ||
}, | ||
"metadata": {}, | ||
"output_type": "display_data" | ||
}, | ||
{ | ||
"data": { | ||
"application/vnd.jupyter.widget-view+json": { | ||
"model_id": "86699bb231414753bfb51786d4a12b7f", | ||
"version_major": 2, | ||
"version_minor": 0 | ||
}, | ||
"text/plain": [ | ||
"Packets: 0/? [00:00<?, ?it/s]" | ||
] | ||
}, | ||
"metadata": {}, | ||
"output_type": "display_data" | ||
}, | ||
{ | ||
"name": "stderr", | ||
"output_type": "stream", | ||
"text": [ | ||
"Atomic Data kurucz_cd23_chianti_H_He already exists in /home/monkhayd/Downloads/tardis-data/kurucz_cd23_chianti_H_He.h5. Will not download - override with force_download=True.\n", | ||
"WARNING: UnitsWarning: 'erg/cm2/s' contains multiple slashes, which is discouraged by the FITS standard [astropy.units.format.generic]\n", | ||
"WARNING:astropy:UnitsWarning: 'erg/cm2/s' contains multiple slashes, which is discouraged by the FITS standard\n", | ||
"/home/monkhayd/Software/tardis/tardis/plasma/properties/radiative_properties.py:93: RuntimeWarning: invalid value encountered in divide\n", | ||
" (g_lower * n_upper) / (g_upper * n_lower)\n", | ||
"/home/monkhayd/Software/tardis/tardis/plasma/properties/radiative_properties.py:93: RuntimeWarning: invalid value encountered in divide\n", | ||
" (g_lower * n_upper) / (g_upper * n_lower)\n" | ||
] | ||
} | ||
], | ||
"source": [ | ||
"import numpy as np\n", | ||
"import matplotlib.pyplot as plt\n", | ||
"from tardis.io.atom_data.util import download_atom_data\n", | ||
"from stardis.base import run_stardis\n", | ||
"from astropy import units as u, constants as const\n", | ||
"\n", | ||
"download_atom_data('kurucz_cd23_chianti_H_He')\n", | ||
"tracing_lambdas = np.mgrid[6540:6590:.01]* u.Angstrom\n", | ||
"\n", | ||
"sim = run_stardis('Tutorial_data/stardis_config_parallel.yml', tracing_lambdas)" | ||
] | ||
} | ||
], | ||
"metadata": { | ||
"kernelspec": { | ||
"display_name": "Python 3", | ||
"language": "python", | ||
"name": "python3" | ||
}, | ||
"language_info": { | ||
"codemirror_mode": { | ||
"name": "ipython", | ||
"version": 3 | ||
}, | ||
"file_extension": ".py", | ||
"mimetype": "text/x-python", | ||
"name": "python", | ||
"nbconvert_exporter": "python", | ||
"pygments_lexer": "ipython3", | ||
"version": "3.11.5" | ||
}, | ||
"orig_nbformat": 4 | ||
}, | ||
"nbformat": 4, | ||
"nbformat_minor": 2 | ||
} |
Oops, something went wrong.