Changeset 2335 for trunk/tsuite
- Timestamp:
- 08/17/08 07:50:08 (5 months ago)
- Location:
- trunk/tsuite/auto
- Files:
-
- 29 modified
- 2 moved
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agn_S_curve_grid.in (modified) (3 diffs)
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aperture_beam_lum.in (modified) (1 diff)
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blr_kk81.in (modified) (1 diff)
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blr_level2.in (modified) (2 diffs)
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coll_coronal.in (modified) (2 diffs)
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coll_heat_only.in (modified) (1 diff)
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coll_t5.in (modified) (1 diff)
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coll_t7.in (modified) (1 diff)
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doc_tsuite.pl (modified) (2 diffs)
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dynamics_orion_flow.in (modified) (1 diff)
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feii_hin.in (modified) (2 diffs)
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feii_hirad.in (modified) (1 diff)
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feii_ste.in (modified) (1 diff)
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func_abund_fluc.in (modified) (2 diffs)
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func_globule.in (modified) (1 diff)
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func_grid_line_ratios.dat (moved) (moved from trunk/tsuite/auto/grid_line_ratios.dat) (1 prop)
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func_grid_line_ratios.in (moved) (moved from trunk/tsuite/auto/grid_line_ratios.in) (1 diff, 1 prop)
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func_hotgas_coolstar.in (modified) (1 diff)
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func_ion_increase.in (modified) (1 diff)
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func_lines.in (modified) (1 diff)
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func_map.in (modified) (1 diff)
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func_set_ion.in (modified) (1 diff)
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func_stopline1.in (modified) (2 diffs)
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func_stopline2.in (modified) (2 diffs)
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func_t3.in (modified) (1 diff)
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func_test.in (modified) (2 diffs)
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func_trans_punch.in (modified) (2 diffs)
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func_trans_read.in (modified) (2 diffs)
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grains_lte.in (modified) (3 diffs)
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grains_temp.in (modified) (1 diff)
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grains_temp_all.in (modified) (1 diff)
Legend:
- Unmodified
- Added
- Removed
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trunk/tsuite/auto/agn_S_curve_grid.in
r1990 r2335 4 4 c this is the generic AGN continuum 5 5 table agn 6 c the ionization parameter 6 c the ionization parameter will be varied 7 7 ionization parameter 0.00 vary 8 8 grid from 0 to 3 in 0.25 dex steps … … 28 28 c line to make line list smaller 29 29 normalize to "totl" 1216 30 print line faint 10 30 print line faint 10 will be varied 31 c create file with list of grid parameters 31 32 punch grid "agn_S_curve_grid.grd" last 33 c save average H+ temperature 32 34 punch average "agn_S_curve_grid.avr" last 33 35 temperature hydrogen 1 34 36 end of temperatures 35 37 punch asserts "agn_S_curve_grid.asr" 38 c save heating and cooling 36 39 punch heating "agn_S_curve_grid.het" last 37 40 punch cooling "agn_S_curve_grid.col" last … … 49 52 c 50 53 51 This is part ofa series of models that check the temperature54 This computes a series of models that check the temperature 52 55 through the S curve in the Fields et al. three-phase model of 53 56 ISM stability. -
trunk/tsuite/auto/aperture_beam_lum.in
r13 r2335 40 40 and when the calculation is complete, the program confirms that the "luminosity" 41 41 of the line is the emitting volume times 1e-10. The aperture command 42 is verified by asserting that th eemission line has the correct "luminosity".42 is verified by asserting that this emission line has the correct "luminosity". 43 43 44 44 -
trunk/tsuite/auto/blr_kk81.in
r2310 r2335 469 469 c 470 470 471 This is the 34standard34BLR model presented by Kwan and Krolik (1981).471 This is the "standard" BLR model presented by Kwan and Krolik (1981). 472 472 473 473 >>refer blr cloud Kwan, J., & Krolik, J. 1981, ApJ, 250, 478 474 474 475 Checks: 475 Compare line intensities to previous versions of CLOUDY 476 by entering into table on page Error! Bookmark not defined.. 476 477 477 - Compare line intensities to previous versions of CLOUDY 478 by entering into table on page Error! Bookmark not defined.. 478 The code caution that the resulting total pressure was not constant 479 is to be expected. The KK calculation assumed constant gas pressure, 480 but internally generature line radiation pressure is significant. 481 Because of this the sum 482 of gas plus radiation pressure was not constant although 483 the gas pressure was. 479 484 480 - A code caution that the resulting total pressure was not constant481 is to be expected. The KK calculation assumed constant gas pressure,482 but radiation pressure was significant. Because of this the sum483 of gas plus radiation pressure was not constant (but gas pressure was).484 -
trunk/tsuite/auto/blr_level2.in
r1998 r2335 1 title test dominant blr_level2 lines1 title test dominant level2 lines 2 2 c 3 3 c commands controlling continuum ========= … … 248 248 c ======================================== 249 249 250 This model checks predictions for the " blr_level2" lines. These are250 This model checks predictions for the "level2" lines. These are 251 251 lines that are normally very weak, have Opacity Project wavelengths, 252 252 and g-bar collision strengths. Phosphorus is given a large abundance 253 so that its blr_level2 lines are significant.253 so that its level2 lines are significant. 254 254 -
trunk/tsuite/auto/coll_coronal.in
r2314 r2335 4 4 c temperature of corona 5 5 coronal equilibrium, 2.5e6 K 6 c assume the sun is a n Atlas atmosphere at 5700K7 blackbody 5770 6 c assume the sun is a blackbody at 5770K 7 blackbody 5770 K 8 8 luminosity solar linear 1 9 9 c … … 297 297 298 298 This is a rough model of the solar corona. 299 The test checks that the table star atlas andcoronal equilibrium commands work.299 The test checks that the coronal equilibrium commands work. 300 300 The gas is predominantly collisionally ionized. 301 301 -
trunk/tsuite/auto/coll_heat_only.in
r1822 r2335 98 98 99 99 This test is an optically thin collisionally ionized gas with no 100 photoionization at all. Before c9601 the code would not do the ionization 101 stage trimming correctly. Original bug caught by Ronnie Hoogerweft. 100 photoionization at all. 102 101 103 102 -
trunk/tsuite/auto/coll_t5.in
r1935 r2335 198 198 199 199 This is a test collisional ionization equilibrium 200 at 1 00000K.200 at 1e5 K. -
trunk/tsuite/auto/coll_t7.in
r1582 r2335 154 154 155 155 Test with only collisional ionization at a 156 high gas hightemperature.156 high temperature. -
trunk/tsuite/auto/doc_tsuite.pl
r13 r2335 149 149 close(THTML); 150 150 151 print "Created:$htests\n $tests\n", ; 151 print "The file $tests contains a list of the file names and titles.\n"; 152 print "The file $htests has the formatted contents of each test case.\n"; 152 153 153 154 … … 166 167 167 168 168 -
trunk/tsuite/auto/dynamics_orion_flow.in
r2181 r2335 132 132 c 133 133 134 This is a model similar in spirit to the blister geometry H IIregion134 This is a model similar in spirit to the blister geometry H+ region 135 135 model computed by Baldwin et al. (1991), but with a D-critical flow. 136 136 Many physical processes have been disabled to make this simulationn faster. -
trunk/tsuite/auto/feii_hin.in
r2314 r2335 7 7 c commands for density & abundances ========= 8 8 hden 18 9 c force a high electron density to insure collisions dominate 9 10 eden 18 10 11 c … … 32 33 This checks that, at high particle densitites, in which 33 34 the gas should be in collisional 34 equilibrium, the level populations of the model Fe+ ion35 equilibrium, the level populations of the large model Fe+ ion 35 36 go to the proper values, where the departure coefficients 36 37 are all equal to unity. -
trunk/tsuite/auto/feii_hirad.in
r2314 r2335 34 34 This checks that, at high radiation densitites, in which 35 35 the gas is irradiated by a blackbody in strict thermodynamic 36 equilibrium, the level populations of the model Fe+ ion36 equilibrium, the level populations of the large model Fe+ ion 37 37 go to the proper values, where the departure coefficients 38 38 are all equal to unity. -
trunk/tsuite/auto/feii_ste.in
r2314 r2335 34 34 This model has a very high iron abundance, 100x H, and most Fe is 35 35 in the form of Fe+. It is irradiated by a blackbody in strict 36 thermodynamic equilibrium. The mode checksthat the temperature36 thermodynamic equilibrium. We check that the temperature 37 37 of the gas is equal to the radiation temperature, to confirm 38 38 that the thermal properties of the model FeII atom obey thermodynamics. -
trunk/tsuite/auto/func_abund_fluc.in
r1092 r2335 1 title this runs the standard, one command, test, which contains many asserts1 title check fluctuating heavy-element abundances 2 2 c commands controlling continuum ========= 3 3 blackbody 5 … … 33 33 c 34 34 35 This checks that the variable abundances option stillworks35 This checks that the variable abundances option works 36 36 -
trunk/tsuite/auto/func_globule.in
r2016 r2335 56 56 57 57 58 This model uses the globule command, andtests that the zoning logic58 This model uses the globule command, tests that the zoning logic 59 59 works for this extreme case, and that the code is able to converge 60 60 the globule model. -
trunk/tsuite/auto/func_grid_line_ratios.dat
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trunk/tsuite/auto/func_grid_line_ratios.in
r2107 r2335 25 25 c 26 26 c commands controlling output ===== 27 punch line list " grid_line_ratios.pun" "grid_line_ratios.dat" ratio no hash28 punch grid " grid_line_ratios.grd"27 punch line list "func_grid_line_ratios.pun" "func_grid_line_ratios.dat" ratio no hash 28 punch grid "func_grid_line_ratios.grd" 29 29 c 30 30 c commands giving (lack of) assert ========== 31 31 assert nothing 0 32 32 c 33 c grid_line_line_ratios.in33 c func_grid_line_line_ratios.in 34 34 c class function 35 35 c =================================================== -
trunk/tsuite/auto/func_hotgas_coolstar.in
r2314 r2335 114 114 c 115 115 116 This is a test where the continuum source is very soft,117 and does not extend into energies where the116 This is a test where the CMB is the only continuum source. 117 It does not extend to energies where the 118 118 code needs to work. There are special cases 119 119 used in this situation, for continuum addressing, -
trunk/tsuite/auto/func_ion_increase.in
r2016 r2335 231 231 c 232 232 233 this model tests the case where the ionization increases with depth. 234 The density is a fast powerlaw to insure this.235 236 237 233 This density falls off faster than 1/r^2 so the ionization increases 234 with depth. Most sims have decreasing rather than increasing ionization. 235 236 237 -
trunk/tsuite/auto/func_lines.in
r888 r2335 35 35 The func_lines lines.dat gives atomic data for all the lines, and their 36 36 critical density at 10000 K. 37 The large H2 and Fe II model atoms are turned on to include their lines. 37 38 -
trunk/tsuite/auto/func_map.in
r1305 r2335 17 17 c 18 18 c commands controlling output ========= 19 c change plot to punchto generate plot for hazy19 c save map information to generate plot for hazy 20 20 punch map file="func_map.dta" 21 21 set nmaps 100 -
trunk/tsuite/auto/func_set_ion.in
r241 r2335 41 41 c ======================================== 42 42 c 43 43 44 this script exercies the option to specify the ionization of a species -
trunk/tsuite/auto/func_stopline1.in
r1532 r2335 14 14 c commands controlling geometry ========= 15 15 c stop calc at line ratio, the point of this test 16 stop line " c2" 157.6m reaches 0.035816 stop line "C 2" 157.6m reaches 0.0358 17 17 c 18 18 c other commands for details ========= … … 32 32 c 33 33 34 this is an example of a simple calculation that stops when34 This is an example of a simple calculation that stops when 35 35 a line reaches a specified intensity. 36 36 The option to turn off elements with trivial abundances is used. -
trunk/tsuite/auto/func_stopline2.in
r1489 r2335 12 12 c commands controlling geometry ========= 13 13 c stop calc at line ratio, the point of this test 14 stop line " c 2" 157.6m reaches 0.002 relative to "o 3" 500714 stop line "C 2" 157.6m reaches 0.002 relative to "o 3" 5007 A 15 15 c 16 16 c other commands for details ========= … … 33 33 34 34 this is an example of a simple calculation that stops when 35 a certain line ratio is reached 35 a certain emission line ratio is reached 36 -
trunk/tsuite/auto/func_t3.in
r2314 r2335 10 10 c commands controlling geometry ========= 11 11 stop zone 1 12 c specify a thin cell of gas -1 cm thick12 c specify a thin cell of gas 1 cm thick 13 13 set dr 0 14 14 c -
trunk/tsuite/auto/func_test.in
r1092 r2335 1 title this runs the standard, one command, test, which contains many asserts1 title run smoke test 2 2 c commands controlling continuum ========= 3 3 test … … 27 27 c 28 28 29 This runs the "test"command, which include several asserts.29 This runs the smoke test command, which include several asserts. 30 30 -
trunk/tsuite/auto/func_trans_punch.in
r2314 r2335 23 23 c 24 24 c commands giving the asserts ========= 25 c this contains a large number of asserts 25 c this contains a large number of asserts that both tests use 26 26 init file "trans.dat" 27 27 c … … 35 35 continuum then read it. 36 36 37 This sim must come before func_trans_read since it 38 generates the punch file needed by func_trans_read. 39 Alphabetical order insures this. -
trunk/tsuite/auto/func_trans_read.in
r2314 r2335 1 1 title second of transpunch/transread pair, used transmitted continuum 2 c the transmitted continuum produced by func_trans_punch "2 c the transmitted continuum produced by func_trans_punch 3 3 c 4 4 c commands controlling continuum ========= … … 19 19 c 20 20 c commands controlling output ========= 21 c this contains a large number of asserts 21 c this contains a large number of asserts used by both commands 22 22 init file "trans.dat" 23 23 print incident continuum -
trunk/tsuite/auto/grains_lte.in
r2260 r2335 4 4 c commands controlling continuum ========= 5 5 black 3 lte 6 //7 6 c 8 7 c commands for density & abundances ========= … … 10 9 eden 5 11 10 init file "hheonly.ini" 12 // need to normalize to some line, Owill provide some11 c need to normalize to some line, oxygen will provide some 13 12 element oxygen on 13 c ism grains with high dust to gas ratio 14 14 grain abund 1 15 15 c … … 54 54 c 55 55 56 This test radiations a set of grains with a true blackbody in56 This test irradiates a set of grains with a true blackbody in 57 57 strict thermodynamic equilibrium. We expect the grains 58 58 (and everything else) to equilibriate at the blackbody temperature. 59 59 The gas temperature is forced to the radiation temperature because 60 60 the current molecule network (based on ISM approximations) does not 61 now go to LTE in the highradiation density limit. The calculation61 go to LTE in the high-radiation density limit. The calculation 62 62 asserts that all grain temperatures are very close to the radiation 63 63 temperature. -
trunk/tsuite/auto/grains_temp.in
r2314 r2335 41 41 c 42 42 43 This turns on all the grain species that the code knows about,44 at least in its default state.A model of an ionized layer is43 This turns on all the grain species that are included in the distribution. 44 A model of an ionized layer is 45 45 done and the asserts confirm the resulting grain temperatures. 46 46 -
trunk/tsuite/auto/grains_temp_all.in
r860 r2335 74 74 c 75 75 76 this is a relatively quick test of the newgrains.76 This is a relatively quick test of grains. 77 77 The Orion and ISM silicate and graphitic grains 78 78 are turned on and their equilibrium temperature 79 checked. This uses distributed grain sizes by default.79 checked.
