{ "cells": [ { "cell_type": "markdown", "metadata": {}, "source": [ "# Changing Parameters" ] }, { "cell_type": "markdown", "metadata": {}, "source": [ "## Import Necessary Code" ] }, { "cell_type": "code", "execution_count": 1, "metadata": {}, "outputs": [ { "data": { "application/vnd.jupyter.widget-view+json": { "model_id": "e718348bdbb54da288b328b5cb237fe0", "version_major": 2, "version_minor": 0 }, "text/plain": [ "Iterations: 0/? [00:00" ] }, "metadata": {}, "output_type": "display_data" } ], "source": [ "tracing_lambdas = np.mgrid[6586:6592:0.01]* u.Angstrom\n", "\n", "\n", "for carbon_rescaling in range(0, 40, 5):\n", " sim = run_stardis('Changing_Param_Example.yml', tracing_lambdas, add_config_dict={'input_model.nuclide_rescaling_dict': {'C' : carbon_rescaling}})\n", " plt.plot(sim.lambdas, sim.spectrum_lambda, alpha = 0.4, label = f\"C rescaling factor: {carbon_rescaling}\")\n", "plt.title(\"STARDIS Solar Spectrum\")\n", "plt.xlabel(r\"Wavelength [$\\AA$]\")\n", "plt.ylabel(r\"Flux density [erg/s/cm$^2$/$\\AA$]\")\n", "plt.tight_layout()\n", "plt.legend()\n", "\n", "plt.show()\n" ] }, { "cell_type": "code", "execution_count": null, "metadata": {}, "outputs": [], "source": [] } ], "metadata": { "kernelspec": { "display_name": "stardis", "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": "3.12.4" } }, "nbformat": 4, "nbformat_minor": 2 }