Commit e15e34d606a7f455b27f44cb45ce7eb6d94c2b15
1 parent
b6361456
Exists in
master
ignored
Showing
1 changed file
with
0 additions
and
345 deletions
Show diff stats
test_plot.py deleted
| ... | ... | @@ -1,345 +0,0 @@ |
| 1 | -# -*- coding: utf-8 -*- | |
| 2 | -""" | |
| 3 | -Created on Sun Jul 17 14:31:57 2022 | |
| 4 | - | |
| 5 | -@author: frede | |
| 6 | -""" | |
| 7 | - | |
| 8 | -import main_program as mp | |
| 9 | -from astropy.table import Table | |
| 10 | -import four_levels_model as four_lvl | |
| 11 | -import matplotlib.pyplot as plt | |
| 12 | -import numpy as np | |
| 13 | - | |
| 14 | -'''================================ initialization of parameters ================================''' | |
| 15 | - | |
| 16 | -filename = './converted/kp00_30000.txt' | |
| 17 | -star_radius = 5 | |
| 18 | -t_gas = 500 | |
| 19 | -n_e = 1.6 | |
| 20 | -n_c = 54 | |
| 21 | -parsec = 6.5e-8 | |
| 22 | -fc_pah = 0.1 | |
| 23 | -ISRF = False | |
| 24 | - | |
| 25 | -# test3 = mp.HeatingGas(filename, star_radius, t_gas, n_e, n_c, parsec, fc_pah, ISRF) | |
| 26 | -# test3.parameters() | |
| 27 | -# test4 = mp.HeatingGas(filename, star_radius, t_gas, n_e, n_c, parsec, fc_pah, ISRF) | |
| 28 | -# test4.parameters() | |
| 29 | - | |
| 30 | -''' parameter ''' | |
| 31 | -distance_list = np.array([parsec]) | |
| 32 | -for j in range(2,1002,1): | |
| 33 | - d = distance_list[0] | |
| 34 | - distance_list = np.append(distance_list, j * d) #in parsec | |
| 35 | - | |
| 36 | -test = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, n_c, parsec, fc_pah, ISRF) | |
| 37 | -test.parameters() | |
| 38 | - | |
| 39 | -# calculus=0 | |
| 40 | -# for i in distance_list: | |
| 41 | -# test = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, n_c, i, fc_pah, ISRF) | |
| 42 | -# test.parameters() | |
| 43 | -# calculus += test.total_gas_heating*1e-7/(test.g_0 * test.heating_efficiency * 0.1) | |
| 44 | - | |
| 45 | -# print('value = ',calculus/len(distance_list)) | |
| 46 | - | |
| 47 | -'''================================ plots ================================''' | |
| 48 | - | |
| 49 | -# ''' intensity per wavelength ''' | |
| 50 | -# plt.figure() | |
| 51 | -# plt.xlim([0,1500]) | |
| 52 | -# plt.plot(test.wavelength,test.wavelength_intensity*1e-3,'k') | |
| 53 | -# plt.ylabel('intensity spectrum (W m$^{-2}$ sr$^{-1}$ nm$^{-1}$)') | |
| 54 | -# plt.xlabel('wavelength (nm)') | |
| 55 | - | |
| 56 | -''' average of 3 sizes categories of pah of photoabsorption sigma | |
| 57 | -and photoionization sigma_ion cross sections per C atom of pahs | |
| 58 | -as functions of photon energy in eV''' | |
| 59 | - | |
| 60 | -''' conversion from mb/C atom to cmยฒ/C atom ''' | |
| 61 | -test.pah_cross_a = test.pah_cross_a*1e-18 | |
| 62 | -test.pah_cross_n = test.pah_cross_n*1e-18 | |
| 63 | -test.pah_cross_c = test.pah_cross_c*1e-18 | |
| 64 | -test.pah_cross_dc = test.pah_cross_dc*1e-18 | |
| 65 | - | |
| 66 | -''' small n_c ''' | |
| 67 | -test_small_n_c_1 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 32, parsec, fc_pah, ISRF) | |
| 68 | -test_small_n_c_2 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 36, parsec, fc_pah, ISRF) | |
| 69 | -test_small_n_c_3 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 38, parsec, fc_pah, ISRF) | |
| 70 | - | |
| 71 | -test_small_n_c_1.parameters() | |
| 72 | -test_small_n_c_2.parameters() | |
| 73 | -test_small_n_c_3.parameters() | |
| 74 | - | |
| 75 | -''' medium n_c ''' | |
| 76 | -test_medium_n_c_1 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 40, parsec, fc_pah, ISRF) | |
| 77 | -test_medium_n_c_2 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 42, parsec, fc_pah, ISRF) | |
| 78 | - | |
| 79 | -test_medium_n_c_1.parameters() | |
| 80 | -test_medium_n_c_2.parameters() | |
| 81 | - | |
| 82 | -''' large n_c ''' | |
| 83 | -test_large_n_c_1 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 48, parsec, fc_pah, ISRF) | |
| 84 | -test_large_n_c_2 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 54, parsec, fc_pah, ISRF) | |
| 85 | -test_large_n_c_3 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, 66, parsec, fc_pah, ISRF) | |
| 86 | - | |
| 87 | -test_large_n_c_1.parameters() | |
| 88 | -test_large_n_c_2.parameters() | |
| 89 | -test_large_n_c_3.parameters() | |
| 90 | - | |
| 91 | -''' average of first and second photoionization yield ''' | |
| 92 | -yield_of_first_photoionization = (test_small_n_c_1.yield_of_first_photoionization +\ | |
| 93 | - test_small_n_c_2.yield_of_first_photoionization +\ | |
| 94 | - test_small_n_c_3.yield_of_first_photoionization +\ | |
| 95 | - test_medium_n_c_1.yield_of_first_photoionization +\ | |
| 96 | - 2*test_medium_n_c_2.yield_of_first_photoionization +\ | |
| 97 | - test_large_n_c_1.yield_of_first_photoionization +\ | |
| 98 | - test_large_n_c_2.yield_of_first_photoionization +\ | |
| 99 | - test_large_n_c_3.yield_of_first_photoionization )/9 | |
| 100 | -yield_of_second_photoionization = (test_small_n_c_1.yield_of_second_photoionization +\ | |
| 101 | - test_small_n_c_2.yield_of_second_photoionization +\ | |
| 102 | - test_small_n_c_3.yield_of_second_photoionization +\ | |
| 103 | - test_medium_n_c_1.yield_of_second_photoionization +\ | |
| 104 | - 2*test_medium_n_c_2.yield_of_second_photoionization +\ | |
| 105 | - test_large_n_c_1.yield_of_second_photoionization +\ | |
| 106 | - test_large_n_c_2.yield_of_second_photoionization +\ | |
| 107 | - test_large_n_c_3.yield_of_second_photoionization )/9 | |
| 108 | - | |
| 109 | -''' average of ionization cross-section for the cases of neutral molecules, and | |
| 110 | -cations ''' | |
| 111 | -ionization_cross_a = test.pah_cross_a * test.detachment_yield | |
| 112 | -ionization_cross_n = test.pah_cross_n * yield_of_first_photoionization | |
| 113 | -ionization_cross_c = test.pah_cross_c * yield_of_second_photoionization | |
| 114 | -#ionization_cross_dc is too small to be traced | |
| 115 | - | |
| 116 | -''' average of energy per cross-section for the cases of neutral molecules, | |
| 117 | -cations and dications ''' | |
| 118 | -energy = (test.energy_negative_charged + test.energy_neutral + test.energy_charged + test.energy_double_charged)/4 | |
| 119 | - | |
| 120 | -''' plot sigma and sigma_ion in cmยฒ/(C atom) as a function of photon energy in eV | |
| 121 | -for the cases of neutral, charged and double charged molecules ''' | |
| 122 | -plt.figure(figsize=(3.57,9.0)) | |
| 123 | - | |
| 124 | -plt.subplot(4,1,1) | |
| 125 | -plt.plot(test.energy_negative_charged,test.pah_cross_a,'k', label='$\sigma(E,Z)$') | |
| 126 | -plt.plot(energy,ionization_cross_a,'k',ls='--', label='$\sigma_{ion}(E,Z)$') | |
| 127 | -plt.title('Z=-1', fontsize = 10) | |
| 128 | -plt.legend(fontsize = 8) | |
| 129 | - | |
| 130 | -plt.subplot(4,1,2) | |
| 131 | -plt.plot(test.energy_neutral,test.pah_cross_n,'k') | |
| 132 | -plt.plot(energy,ionization_cross_n,'k',ls='--') | |
| 133 | -plt.title('Z=0', fontsize = 10) | |
| 134 | - | |
| 135 | -plt.subplot(4,1,3) | |
| 136 | -plt.plot(test.energy_neutral,test.pah_cross_c,'k') | |
| 137 | -plt.plot(energy,ionization_cross_c,'k',ls='--') | |
| 138 | -plt.title('Z=1', fontsize = 10) | |
| 139 | -plt.ylabel('Cross sections (cm$^2$/C)') | |
| 140 | - | |
| 141 | -plt.subplot(4,1,4) | |
| 142 | -plt.plot(test.energy_neutral,test.pah_cross_dc,'k') | |
| 143 | -plt.title('Z=2', fontsize = 10) | |
| 144 | -plt.xlabel('Photon energy (eV)') | |
| 145 | - | |
| 146 | -plt.subplots_adjust(hspace = 0.35) | |
| 147 | -plt.savefig('cross_ioni_section_categories.pdf', bbox_inches='tight') | |
| 148 | -if ISRF == False: | |
| 149 | - | |
| 150 | - ''' evolution of the different populations of neutral pah molecules, | |
| 151 | - # cations and dications as a function of the distance to the star considered ''' | |
| 152 | - | |
| 153 | - ''' parameter ''' | |
| 154 | - # population_frac3 = np.zeros([1, len(distance_list)]) | |
| 155 | - # population_frac4 = np.zeros([4, len(distance_list)]) | |
| 156 | - | |
| 157 | - ''' indentation ''' | |
| 158 | - # j=0 | |
| 159 | - # gamma_list3 = [] | |
| 160 | - # gamma_list4 = [] | |
| 161 | - # for i in distance_list: | |
| 162 | - # population_plot_test3 = mp.HeatingGas(filename, star_radius, t_gas, n_e, n_c, i, fc_pah, ISRF) | |
| 163 | - # population_plot_test3.parameters() | |
| 164 | - # population_frac3[0,j] =(population_plot_test3.frac_charged +\ | |
| 165 | - # population_plot_test3.frac_double_charged)/\ | |
| 166 | - # (population_plot_test3.frac_neutral +\ | |
| 167 | - # population_plot_test3.frac_charged +\ | |
| 168 | - # population_plot_test3.frac_double_charged) | |
| 169 | - # # population_frac3[0,j] = population_plot_test3.frac_neutral | |
| 170 | - # # population_frac3[1,j] = population_plot_test3.frac_charged | |
| 171 | - # # population_frac3[2,j] = population_plot_test3.frac_double_charged | |
| 172 | - # gamma_list3.append(population_plot_test3.gamma) | |
| 173 | - | |
| 174 | - # population_plot_test4 = four_lvl.HeatingGas(filename, star_radius, t_gas, n_e, n_c, i, fc_pah, ISRF) | |
| 175 | - # population_plot_test4.parameters() | |
| 176 | - # population_frac4[0,para] =(population_plot_test4.frac_anion +\ | |
| 177 | - # population_plot_test4.frac_charged +\ | |
| 178 | - # population_plot_test4.frac_double_charged)/\ | |
| 179 | - # (population_plot_test4.frac_anion +\ | |
| 180 | - # population_plot_test4.frac_neutral +\ | |
| 181 | - # population_plot_test4.frac_charged +\ | |
| 182 | - # population_plot_test4.frac_double_charged) | |
| 183 | - # population_frac4[0,j] = population_plot_test4.frac_anion | |
| 184 | - # population_frac4[1,j] = population_plot_test4.frac_neutral | |
| 185 | - # population_frac4[2,j] = population_plot_test4.frac_charged | |
| 186 | - # population_frac4[3,j] = population_plot_test4.frac_double_charged | |
| 187 | - # gamma_list4.append(population_plot_test4.gamma) | |
| 188 | - # j=j+1 | |
| 189 | - | |
| 190 | - ''' population fractions as function of the distance ''' | |
| 191 | - # plt.figure(figsize=(5.90,3.93)) | |
| 192 | - # plt.plot(gamma_list3,population_frac3[0,:],c='k',label='3 levels model') | |
| 193 | - # plt.plot(gamma_list4,population_frac4[0,:],ls='--', c='k',label='4 levels model') | |
| 194 | - # plt.xlim([1e1, 1e7]) | |
| 195 | - # plt.plot(gamma_list3, population_frac3[0,:], color = 'green', label='Z=0, 3 levels model') | |
| 196 | - # plt.plot(gamma_list3, population_frac3[1,:], color = 'blue', label='Z=1, 3 levels model') | |
| 197 | - # plt.plot(gamma_list3, population_frac3[2,:], color = 'red', label='Z=2, 3 levels model') | |
| 198 | - # plt.plot(gamma_list4, population_frac4[0,:], ls='--', color = 'k', label='Z=-1, 4 levels model') | |
| 199 | - # plt.plot(gamma_list4, population_frac4[1,:], ls='--', color = 'green', label='Z=0, 4 levels model') | |
| 200 | - # plt.plot(gamma_list4, population_frac4[2,:], ls='--', color = 'k', label='Z=1, 4 levels model') | |
| 201 | - # plt.plot(gamma_list4, population_frac4[3,:], ls='--', color = 'red', label='Z=2, 4 levels model') | |
| 202 | - # plt.plot(gamma_list3, population_frac3[0,:]+population_frac3[1,:]+population_frac3[2,:],'blue') | |
| 203 | - # plt.plot(gamma_list4, population_frac4[0,:]+population_frac4[1,:]+population_frac4[2,:]+population_frac4[3,:],'darkblue') | |
| 204 | - # plt.xlabel('$\gamma$ ($G_0\sqrt{T}/n_e$)') | |
| 205 | - # plt.ylabel('population fraction R$_i$') | |
| 206 | - # plt.legend() | |
| 207 | - | |
| 208 | - ''' photoelectric efficiencies with the pah heating model ''' | |
| 209 | - | |
| 210 | - # gamma_list_T_one3 = [] | |
| 211 | - # heating_efficiency_list_T_one3 = [] | |
| 212 | - | |
| 213 | - # gamma_list_T_two3 = [] | |
| 214 | - # heating_efficiency_list_T_two3 = [] | |
| 215 | - | |
| 216 | - # gamma_list_T_one4 = [] | |
| 217 | - # heating_efficiency_list_T_one4 = [] | |
| 218 | - | |
| 219 | - # gamma_list_T_two4 = [] | |
| 220 | - # heating_efficiency_list_T_two4 = [] | |
| 221 | - | |
| 222 | - # ratio1_1 = [] | |
| 223 | - # ratio2_1 = [] | |
| 224 | - # gamma_mean1_1 = [] | |
| 225 | - # gamma_mean2_1 = [] | |
| 226 | - # gamma_list_1 = [] | |
| 227 | - # j = 0 | |
| 228 | - # for i in distance_list: | |
| 229 | - # j = j+1 | |
| 230 | - # if j%100 == 0: | |
| 231 | - # print('Progression ร {}'.format(j/10),'%') | |
| 232 | - # print('') | |
| 233 | - # test_for_efficiencies_T_one3 = mp.HeatingGas(filename, star_radius, 100, n_e, 54, i, fc_pah, ISRF) | |
| 234 | - # test_for_efficiencies_T_one3.parameters() | |
| 235 | - # gamma_list_T_one3.append(test_for_efficiencies_T_one3.gamma) | |
| 236 | - # heating_efficiency_list_T_one3.append(test_for_efficiencies_T_one3.heating_efficiency) | |
| 237 | - | |
| 238 | - # test_for_efficiencies_T_two3 = mp.HeatingGas(filename, star_radius, 1000, n_e, 54, i, fc_pah, ISRF) | |
| 239 | - # test_for_efficiencies_T_two3.parameters() | |
| 240 | - # gamma_list_T_two3.append(test_for_efficiencies_T_two3.gamma) | |
| 241 | - # heating_efficiency_list_T_two3.append(test_for_efficiencies_T_two3.heating_efficiency) | |
| 242 | - | |
| 243 | - # test_for_efficiencies_T_one4 = four_lvl.HeatingGas(filename, star_radius, 100, n_e, n_c, i, fc_pah, ISRF) | |
| 244 | - # test_for_efficiencies_T_one4.parameters() | |
| 245 | - # gamma_list_T_one4.append(test_for_efficiencies_T_one4.gamma) | |
| 246 | - # heating_efficiency_list_T_one4.append(test_for_efficiencies_T_one4.heating_efficiency) | |
| 247 | - | |
| 248 | - # test_for_efficiencies_T_two4 = four_lvl.HeatingGas(filename, star_radius, 1000, n_e, n_c, i, fc_pah, ISRF) | |
| 249 | - # test_for_efficiencies_T_two4.parameters() | |
| 250 | - # gamma_list_T_two4.append(test_for_efficiencies_T_two4.gamma) | |
| 251 | - # heating_efficiency_list_T_two4.append(test_for_efficiencies_T_two4.heating_efficiency) | |
| 252 | - | |
| 253 | - # ratio1_1.append( (test_for_efficiencies_T_one3.heating_efficiency/test_for_efficiencies_T_one4.heating_efficiency)*100) | |
| 254 | - # ratio2_1.append( (test_for_efficiencies_T_two3.heating_efficiency/test_for_efficiencies_T_two4.heating_efficiency)*100) | |
| 255 | - # gamma_mean1_1.append( (test_for_efficiencies_T_one3.gamma + test_for_efficiencies_T_one4.gamma)/2 ) | |
| 256 | - # gamma_mean2_1.append( (test_for_efficiencies_T_two3.gamma + test_for_efficiencies_T_two4.gamma)/2 ) | |
| 257 | - | |
| 258 | - # plt.figure() | |
| 259 | - # plt.xlim([1e1, 1e6]) | |
| 260 | - # plt.loglog(gamma_mean1_1, ratio1_1, 'blue', label='ratio of 3 and 4 levels model $\epsilon_{PAH}$ (T = 100K) ') | |
| 261 | - # plt.loglog(gamma_mean2_1, ratio2_1, 'red', ls='--' , label='ratio of 3 and 4 levels model $\epsilon_{PAH}$ (T = 1000K)') | |
| 262 | - # plt.loglog(gamma_list_T_one3, heating_efficiency_list_T_one3, 'blue', label='$\epsilon_{PAH}$ (T = 100K) 3 levels model') | |
| 263 | - # plt.loglog(gamma_list_T_two3, heating_efficiency_list_T_two3, 'red', ls='--' , label='$\epsilon_{PAH}$ (T = 1000K) 3 levels model') | |
| 264 | - # plt.loglog(gamma_list_T_one4, heating_efficiency_list_T_one4, 'darkblue', label='$\epsilon_{PAH}$ (T = 100K) 4 levels model') | |
| 265 | - # plt.loglog(gamma_list_T_two4, heating_efficiency_list_T_two4, 'darkred', ls='--' , label='$\epsilon_{PAH}$ (T = 1000K) 4 levels model') | |
| 266 | - # plt.xlabel('$\gamma(G_0\sqrt{T}/n_e)$') | |
| 267 | - # plt.ylabel('$\epsilon_{PAH}$') | |
| 268 | - # plt.ylabel('$\epsilon_{PAH, 3lvlmod}$ / $\epsilon_{PAH, 4lvlmod}$ (%)') | |
| 269 | - # plt.legend() | |
| 270 | - | |
| 271 | - # ''' Total photoelectric heating rates of the gas ''' | |
| 272 | - | |
| 273 | - # gamma_list_fc_one3 = [] | |
| 274 | - # total_gas_heating_per_rf_list_fc_one3 = [] | |
| 275 | - | |
| 276 | - # gamma_list_fc_two3 = [] | |
| 277 | - # total_gas_heating_per_rf_list_fc_two3 = [] | |
| 278 | - | |
| 279 | - # gamma_list_fc_one4 = [] | |
| 280 | - # total_gas_heating_per_rf_list_fc_one4 = [] | |
| 281 | - | |
| 282 | - # gamma_list_fc_two4 = [] | |
| 283 | - # total_gas_heating_per_rf_list_fc_two4 = [] | |
| 284 | - | |
| 285 | - # ratio1_2 = [] | |
| 286 | - # ratio2_2 = [] | |
| 287 | - # gamma_mean1_2 = [] | |
| 288 | - # gamma_mean2_2 = [] | |
| 289 | - # Table_list_g_fc5 = [] | |
| 290 | - # Table_list_Gpg0_fc5 = [] | |
| 291 | - | |
| 292 | - # Table_list_g_fc10 = [] | |
| 293 | - # Table_list_Gpg0_fc10 = [] | |
| 294 | - | |
| 295 | - # for i in distance_list: | |
| 296 | - # test_for_total_heating_rates_fc_one3 = mp.HeatingGas(filename, star_radius, t_gas, n_e, n_c, i, 0.05, ISRF) | |
| 297 | - # test_for_total_heating_rates_fc_one3.parameters() | |
| 298 | - # gamma_list_fc_one3.append(test_for_total_heating_rates_fc_one3.gamma) | |
| 299 | - # total_gas_heating_per_rf_list_fc_one3.append( (test_for_total_heating_rates_fc_one3.total_gas_heating*1e-7) / test_for_total_heating_rates_fc_one3.g_0) | |
| 300 | - | |
| 301 | - # test_for_total_heating_rates_fc_two3 = mp.HeatingGas(filename, star_radius, t_gas, n_e, n_c, i, 0.1, ISRF) | |
| 302 | - # test_for_total_heating_rates_fc_two3.parameters() | |
| 303 | - # gamma_list_fc_two3.append(test_for_total_heating_rates_fc_two3.gamma) | |
| 304 | - # total_gas_heating_per_rf_list_fc_two3.append( (test_for_total_heating_rates_fc_two3.total_gas_heating*1e-7) / test_for_total_heating_rates_fc_two3.g_0) | |
| 305 | - | |
| 306 | - # test_for_total_heating_rates_fc_one4 = four_lvl.HeatingGas(filename, star_radius, 500, n_e, 54, i, 0.05, ISRF) | |
| 307 | - # test_for_total_heating_rates_fc_one4.parameters() | |
| 308 | - # gamma_list_fc_one4.append(test_for_total_heating_rates_fc_one4.gamma) | |
| 309 | - # total_gas_heating_per_rf_list_fc_one4.append( (test_for_total_heating_rates_fc_one4.total_gas_heating*1e-7) / test_for_total_heating_rates_fc_one4.g_0) | |
| 310 | - | |
| 311 | - # test_for_total_heating_rates_fc_two4 = four_lvl.HeatingGas(filename, star_radius, 500, n_e, 54, i, 0.1, ISRF) | |
| 312 | - # test_for_total_heating_rates_fc_two4.parameters() | |
| 313 | - # gamma_list_fc_two4.append(test_for_total_heating_rates_fc_two4.gamma) | |
| 314 | - # total_gas_heating_per_rf_list_fc_two4.append( (test_for_total_heating_rates_fc_two4.total_gas_heating*1e-7) / test_for_total_heating_rates_fc_two4.g_0) | |
| 315 | - | |
| 316 | - # ratio1_2.append( ( ( (test_for_total_heating_rates_fc_one3.total_gas_heating*1e-7) /\ | |
| 317 | - # test_for_total_heating_rates_fc_one3.g_0) /\ | |
| 318 | - # ( (test_for_total_heating_rates_fc_one4.total_gas_heating*1e-7) /\ | |
| 319 | - # test_for_total_heating_rates_fc_one4.g_0) )*100 ) | |
| 320 | - # ratio2_2.append( ( ( (test_for_total_heating_rates_fc_two3.total_gas_heating*1e-7) /\ | |
| 321 | - # test_for_total_heating_rates_fc_two3.g_0) /\ | |
| 322 | - # ( (test_for_total_heating_rates_fc_two4.total_gas_heating*1e-7) /\ | |
| 323 | - # test_for_total_heating_rates_fc_two4.g_0) )*100 ) | |
| 324 | - # gamma_mean1_2.append( (test_for_total_heating_rates_fc_one3.gamma+test_for_total_heating_rates_fc_one4.gamma)/2 ) | |
| 325 | - # gamma_mean2_2.append( (test_for_total_heating_rates_fc_two3.gamma+test_for_total_heating_rates_fc_two4.gamma)/2 ) | |
| 326 | - | |
| 327 | - # plt.figure() | |
| 328 | - # plt.xlim([1e1, 1e7]) | |
| 329 | - # plt.loglog(gamma_mean1_2,ratio1_2, 'red', label='ratio of 3 and 4 levels model $\Gamma_{tot}$ (5% of C in PAHs)') | |
| 330 | - # plt.loglog(gamma_mean2_2,ratio2_2, 'blue', label='ratio of 3 and 4 levels model $\Gamma_{tot}$ (10% of C in PAHs)') | |
| 331 | - # plt.loglog(gamma_list_fc_one3, total_gas_heating_per_rf_list_fc_one3, c='red', label='This work (5% of C in PAHs) 3 levels model') | |
| 332 | - # plt.loglog(gamma_list_fc_two3, total_gas_heating_per_rf_list_fc_two3,ls='--', c='blue', label='This work (10% of C in PAHs) 3 levels model') | |
| 333 | - # plt.loglog(gamma_list_fc_one4, total_gas_heating_per_rf_list_fc_one4, c='darkred', label='This work (5% of C in PAHs) 4 levels model') | |
| 334 | - # plt.loglog(gamma_list_fc_two4, total_gas_heating_per_rf_list_fc_two4,ls='--', c='darkblue', label='This work (10% of C in PAHs) 4 levels model') | |
| 335 | - # plt.xlabel('$\gamma(G_0\sqrt{T}/n_e)$') | |
| 336 | - # # plt.ylabel('$\Gamma_{tot}$ (W H$^{-1}$ G$_0^{-1}$)') | |
| 337 | - # plt.ylabel('$\Gamma_{tot, 3lvlmod}$ / $\Gamma_{tot, 4lvlmod}$ (%)') | |
| 338 | - # plt.legend() | |
| 339 | - | |
| 340 | - # Table_values.append(heating_efficiency_list_T_one4) | |
| 341 | - # Table_list_g_fc5 = gamma_list_fc_one4[::-1] | |
| 342 | - # Table_list_Gpg0_fc5 = total_gas_heating_per_rf_list_fc_one4[::-1] | |
| 343 | - | |
| 344 | - # Table_list_g_fc10 = gamma_list_fc_two4[::-1] | |
| 345 | - # Table_list_Gpg0_fc10 = total_gas_heating_per_rf_list_fc_two4[::-1] | |
| 346 | 0 | \ No newline at end of file |