Changeset 14395


Ignore:
Timestamp:
2022-04-12T02:25:01Z (4 months ago)
Author:
marios
Message:

Update docs and tsuite in prep for release

Location:
branches/c17_branch
Files:
5 edited

Legend:

Unmodified
Added
Removed
  • branches/c17_branch/docs/LineLabels.out

    r14383 r14395  
    1                                              Cloudy (c17_branch, r14380, prerelease)
     1                                             Cloudy (c17_branch, r14393, prerelease)
    22                                                         www.nublado.org
    33
     
    886886
    887887
    888                        ********************> Cloudy (c17_branch, r14380, prerelease) <********************
     888                       ********************> Cloudy (c17_branch, r14393, prerelease) <********************
    889889                       * Title Produce report of species labels, data sources, and line wavelengths.     *
    890890                       * # this runs the smoke test, needed in order to set up the species               *
     
    24332433     Mean Jeans  l(cm)5.13E+19  M(sun)8.48E+05  smallest:     len(cm):5.13E+19  M(sun):8.48E+05  a_ox tran: -1.41
    24342434 Rion:1.000E+30  Dist:0.00E+00  Diam:0.000E+00
    2435  Hatom level 70  HatomType: add  HInducImp  F  He tot level: 63  He2 level:   70  ExecTime     6.9
     2435 Hatom level 70  HatomType: add  HInducImp  F  He tot level: 63  He2 level:   70  ExecTime     5.2
    24362436 ConvrgError(%)  <eden>  0.008  MaxEden  0.010  <H-C>  84.59  Max(H-C)   84.59  <Press>   0.000  MaxPrs er  0.000
    24372437  Continuity(%)  chng Te   0.0  elec den   0.0  n(H2)    0.0  n(CO)        0.0
     
    27312731----------------------------------------------------
    27322732
    2733 =============Results of monitors: Cloudy (c17_branch, r14380, prerelease) Thu Oct 21 16:01:20 2021
     2733=============Results of monitors: Cloudy (c17_branch, r14393, prerelease) Mon Apr 11 21:56:38 2022
    27342734 No errors were found.  Summary follows.
    27352735                   Label                   line    computed     asserted Rel Err Set err  type         
     
    27472747 ChkMonitor        htot                       0   -15.0154 =   -15.0190  -0.008   0.050           
    27482748 
    2749  Cloudy compiled on Oct 21 2021 in OS Linux (AMD64) using the g++ 40805 compiler. Mode I32LP64, denormalized float: F double: F.
    2750 
    2751  Cloudy ends: 2 zones, 1 iteration. (single thread) ExecTime(s) 6.91
     2749 Cloudy compiled on Apr 11 2022 in OS Linux (AMD64) using the g++ 40805 compiler. Mode I32LP64, denormalized float: F double: F.
     2750
     2751 Cloudy ends: 2 zones, 1 iteration. (single thread) ExecTime(s) 5.26
    27522752 [Stop in cdMain at maincl.cpp:496, Cloudy exited OK]
  • branches/c17_branch/others.txt

    r14388 r14395  
    44Nick Abel
    55Yago Ascasibar
     6Robert Bauman
    67Manuel Bautista
    78Kevin Blagrave
  • branches/c17_branch/tsuite/auto/doc_tsuite.htm

    r11780 r14395  
    324324<br>save performance "agn_S_curve_grid.per"
    325325<br>save grid "agn_S_curve_grid.grd" last no hash
     326<br>save species densities "agn_S_curve_grid.sden" "Si+12[10:11]" last no hash
    326327<br># save average H+ temperature
    327328<br>save average "agn_S_curve_grid.avr" last no hash
     
    410411<br># commands controlling output    =========
    411412<br>print line column
    412 <br>normallize "Fe26"      1.78177A
     413<br>normallize "Fe26"      1.77982A
    413414<br>plot continuum range 1 1000
    414415<br>save overview ".ovr"
     
    16561657<br>#
    16571658<br># commands controlling output    =========
    1658 <br>normalize to "o  8" 18.9709A
     1659<br>normalize to "o  8" 18.9689A
    16591660<br>save overview "coll_coronal.ovr"
    16601661<br>save performance "coll_coronal.per"
     
    17581759<br># add component of cosmic rays to drive chemistry
    17591760<br>cosmic ray background
    1760 <br>abundances ISM
     1761<br># >>chng 20 sep 19 test updated ISM abundances
     1762<br>abundances "ISM-HD20.abn"
    17611763<br>set H2 Jura rate
    17621764<br>#
     
    19211923<br># other commands for details     =========
    19221924<br>#
    1923 <br>normalize to "o  8" 18.9709A
     1925<br>normalize to "o  8" 18.9689A
    19241926<br># commands controlling output    =========
    19251927<br>save performance "coll_t7.per"
     
    27172719</I></h2><kbd><br>title test the 'list' keyword on the grid command
    27182720<br>blackbody 10000 STE vary
    2719 <br>grid list "func_grid_list.dat" linear
     2721<br>grid list "func_grid_list.dat" linear sequential
    27202722<br>hden 5
    27212723<br>stop zone 1
     
    30213023 
    30223024this script exercies the option to specify the ionization of a species
     3025</p><hr><kbd><h2>func_stopcol.in</h2>  </kbd><h2><I>test stop column density "species" command
     3026</I></h2><kbd><br>title test stop column density "species" command
     3027<br>#
     3028<br># commands controlling continuum =========
     3029<br>ionization parameter -2
     3030<br>blackbody 50000
     3031<br>#
     3032<br># commands for density & abundances =========
     3033<br>hden 2
     3034<br>init file "ism.ini"
     3035<br># test option to turn off elements with small abundances
     3036<br>element limit off -5
     3037<br>#
     3038<br># commands controlling geometry  =========
     3039<br># stop calc at line ratio, the point of this test
     3040<br>stop column density "N+2" 10.
     3041<br>#
     3042<br># other commands for details     =========
     3043<br>constant temperature 10000 K
     3044<br>#
     3045<br># commands controlling output    =========
     3046<br>set save prefix "func_stopcol"
     3047<br>save overview ".ovr"
     3048<br>save performance ".per"
     3049<br>save dr ".dr" last
     3050<br>#
     3051<br>#
     3052<br>#
     3053<br>#
     3054<br># func_stopcol.in
     3055<br># class function
     3056<br># ========================================
     3057<br>#
     3058</kbd><p>
     3059This is an example of a simple calculation that stops when
     3060a column density of a species reaches a specific value.
     3061The tricky part is that the species label contains a number, so
     3062we need to ascertain that the column density is parsed correctly.
    30233063</p><hr><kbd><h2>func_stopline1.in</h2>  </kbd><h2><I>test stop line command
    30243064</I></h2><kbd><br>title test stop line command
     
    33913431<p>
    33923432<p>
     3433</p><hr><kbd><h2>func_trans_lumi.in</h2>  </kbd><h2><I>test transmitted continuum in luminosity mode
     3434</I></h2><kbd><br>title test transmitted continuum in luminosity mode
     3435<br>#
     3436<br># common commands
     3437<br>init file "func_trans_lumi.dat"
     3438<br>#
     3439<br># commands controlling geometry  =========
     3440<br>radius 21
     3441<br>#
     3442<br># commands controlling output    =========
     3443<br>set save prefix "func_trans_lumi"
     3444<br>save overview ".ovr"
     3445<br>save performance ".per"
     3446<br>save ionization last ".ion"
     3447<br>save continuum last ".con"
     3448<br>#
     3449<br># this contains a large number of asserts that both tests use
     3450<br>init file "trans_lumi.dat"
     3451<br>#
     3452<br># func_trans_lumi.in
     3453<br># class function
     3454<br># ========================================
     3455<br>#
     3456</kbd><p>
     3457func_trans_lumi, func_trans_save_lumi, and func_trans_read_lumi_scale are a
     3458set of tests that check that the code can save a transmitted continuum in
     3459luminosity mode and then read it back in.
     3460<p>
     3461func_trans_lumi.in: this sim is directly illuminated by a BB at Rin = 1e21.
     3462  Its predictions should be identical to func_trans_read_lumi_scale.in.
     3463<p>
     3464func_trans_save_lumi.in: this sim is directly illuminated by a BB at Rin =
     3465  1e20. It saves the transmitted continuum and has no monitors.
     3466<p>
     3467func_trans_read_lumi_scale.in: this sim is illiminated by the transmitted
     3468  continuum at Rin = 1e21. Its predictions should be almost identical to
     3469  func_trans_lumi.in. This tests that the transmitted continuum works
     3470  correctly in luminosity mode and also that spherical dilution is handled
     3471  correctly.
    33933472</p><hr><kbd><h2>func_trans_read.in</h2>  </kbd><h2><I>second of func_trans_save/func_trans_read pair, use transmitted continuum
    33943473</I></h2><kbd><br>title second of func_trans_save/func_trans_read pair, use transmitted continuum
     
    34283507continuum then read it.
    34293508<p>
     3509</p><hr><kbd><h2>func_trans_read_lumi_scale.in</h2>  </kbd><h2><I>test read transmitted continuum in luminosity mode
     3510</I></h2><kbd><br>title test read transmitted continuum in luminosity mode
     3511<br>#
     3512<br># commands controlling continuum =========
     3513<br>table read "func_trans_save_lumi.trn" scale
     3514<br># second, very faint SED to force luminosity mode
     3515<br>blackbody 50
     3516<br>luminosity 1
     3517<br>#
     3518<br># commands for density & abundances =========
     3519<br>hden 3
     3520<br>#
     3521<br># commands controlling geometry  =========
     3522<br>radius 21
     3523<br>set dr 0
     3524<br>stop zone 1
     3525<br>#
     3526<br># other commands for details     =========
     3527<br>iterate
     3528<br>#
     3529<br># commands controlling output    =========
     3530<br>set save prefix "func_trans_read_lumi_scale"
     3531<br>save overview ".ovr"
     3532<br>save performance ".per"
     3533<br>save ionization last ".ion"
     3534<br>save continuum last ".con"
     3535<br>#
     3536<br># this contains a large number of asserts that both tests use
     3537<br>init file "trans_lumi.dat"
     3538<br>#
     3539<br># func_trans_read_lumi_scale.in
     3540<br># class function
     3541<br># ========================================
     3542<br>#
     3543</kbd><p>
     3544func_trans_lumi, func_trans_save_lumi, and func_trans_read_lumi_scale are a
     3545set of tests that check that the code can save a transmitted continuum in
     3546luminosity mode and then read it back in.
     3547<p>
     3548func_trans_lumi.in: this sim is directly illuminated by a BB at Rin = 1e21.
     3549  Its predictions should be identical to func_trans_read_lumi_scale.in.
     3550<p>
     3551func_trans_save_lumi.in: this sim is directly illuminated by a BB at Rin =
     3552  1e20. It saves the transmitted continuum and has no monitors.
     3553<p>
     3554func_trans_read_lumi_scale.in: this sim is illiminated by the transmitted
     3555  continuum at Rin = 1e21. Its predictions should be almost identical to
     3556  func_trans_lumi.in. This tests that the transmitted continuum works
     3557  correctly in luminosity mode and also that spherical dilution is handled
     3558  correctly.
     3559<p>
     3560This sim must come after func_trans_save_lumi since it needs the save file
     3561generated by func_trans_save_lumi.
    34303562</p><hr><kbd><h2>func_trans_read_scale.in</h2>  </kbd><h2><I>second of func_trans_save/func_trans_readread pair
    34313563</I></h2><kbd><br>title second of func_trans_save/func_trans_readread pair
     
    35143646generates the save file needed by func_trans_read.
    35153647Alphabetical order insures this.
     3648</p><hr><kbd><h2>func_trans_save_lumi.in</h2>  </kbd><h2><I>test save transmitted continuum in luminosity mode
     3649</I></h2><kbd><br>title test save transmitted continuum in luminosity mode
     3650<br>#
     3651<br># common commands
     3652<br>init file "func_trans_lumi.dat"
     3653<br>#
     3654<br># commands controlling geometry  =========
     3655<br>radius 20
     3656<br>#
     3657<br># commands controlling output    =========
     3658<br>set save prefix "func_trans_save_lumi"
     3659<br>save overview ".ovr"
     3660<br>save performance ".per"
     3661<br>save ionization last ".ion"
     3662<br>save continuum last ".con"
     3663<br>save transmitted continuum ".trn"
     3664<br>#
     3665<br>#
     3666<br># func_trans_save_lumi.in
     3667<br># class function
     3668<br># ========================================
     3669<br>#
     3670</kbd><p>
     3671func_trans_lumi, func_trans_save_lumi, and func_trans_read_lumi_scale are a
     3672set of tests that check that the code can save a transmitted continuum in
     3673luminosity mode and then read it back in.
     3674<p>
     3675func_trans_lumi.in: this sim is directly illuminated by a BB at Rin = 1e21.
     3676  Its predictions should be identical to func_trans_read_lumi_scale.in.
     3677<p>
     3678func_trans_save_lumi.in: this sim is directly illuminated by a BB at Rin =
     3679  1e20. It saves the transmitted continuum and has no monitors.
     3680<p>
     3681func_trans_read_lumi_scale.in: this sim is illiminated by the transmitted
     3682  continuum at Rin = 1e21. Its predictions should be almost identical to
     3683  func_trans_lumi.in. This tests that the transmitted continuum works
     3684  correctly in luminosity mode and also that spherical dilution is handled
     3685  correctly.
     3686<p>
     3687This sim must come before func_trans_read_lumi_scale since it generates the
     3688save file needed by func_trans_read_lumi_scale.
    35163689</p><hr><kbd><h2>grains_hot.in</h2>  </kbd><h2><I>test temperature of gas and dust in high energy density environment
    35173690</I></h2><kbd><br>title test temperature of gas and dust in high energy density environment
     
    35353708<br>#
    35363709<br># commands controlling output    =========
    3537 <br>normalize to "O  8" 18.9709A
     3710<br>normalize to "O  8" 18.9689A
    35383711<br>save performance "grains_hot.per"
    35393712<br>save overview "grains_hot.ovr" last
     
    35713744<br>#
    35723745<br># commands controlling output    =========
    3573 <br>normalize to "O  8" 18.9709A
     3746<br>normalize to "O  8" 18.9689A
    35743747<br>save performance "grains_hot_wd01.per"
    35753748<br>save overview "grains_hot_wd01.ovr" last
     
    46944867<br>save performance "h_t4_conemis.per"
    46954868<br>save continuum "h_t4_conemis.con" last no title units microns
    4696 <br>save spectrum "h_t4_conemis.ncon" last no title units microns
    46974869<br>#
    46984870<br># h_t4_conemis.in
     
    47364908<br>save continuum "h_t4_conemis_lon.con" last units microns
    47374909<br>save two photon continuum "h_t4_conemis_lon.2nu" last rydbergs
    4738 <br>save spectrum "h_t4_conemis_lon.ncon" last units microns
    47394910<br>#
    47404911<br># h_t4_conemis_lon.in
     
    48315002<br>save overview "heatomt10.ovr"
    48325003<br>save performance "heatomt10.per"
    4833 <br>save spectrum  "heatomt10.spc" last no title units microns
    48345004<br>save continuum "heatomt10.con" last no title units microns
    48355005<br>save diffuse continuum "heatomt10.dif" last no title units microns
     
    48795049<br>save diffuse continuum "heatomt10lon.dif" last units microns
    48805050<br>save two photon continuum "heatomt10lon.2nu" last
    4881 <br>save spectrum "heatomt10lon.ncon" last units microns
    48825051<br>#
    48835052<br># heatomt10lon.in
     
    49165085<br>save performance "heiont10.per"
    49175086<br>save continuum "heiont10.con" last no title units microns
    4918 <br>save spectrum  "heiont10.spc" last no title units microns
    49195087<br>#
    49205088<br># heiont10.in
     
    97879955<p>
    97889956<p>
     9957</p><hr><kbd><h2>lya-21cm-constant.in</h2>  </kbd><h2><I>test effect of lya pump on spin temperature
     9958</I></h2><kbd><br>title test effect of lya pump on spin temperature
     9959<br>#
     9960<br># commands controlling continuum =========
     9961<br>#
     9962<br>table ism
     9963<br>extinguish column 22
     9964<br>CMB, z=0
     9965<br>#
     9966<br># commands for density & abundances =========
     9967<br># set the density and composition, ism with grains
     9968<br>#
     9969<br>hden 2
     9970<br>abundance ism
     9971<br>#
     9972<br># other commands for details     =========
     9973<br>#
     9974<br># this is an important ionization source
     9975<br>cosmic rays background 
     9976<br># optical depth
     9977<br>double
     9978<br>iterate
     9979<br>turbulence 3 km/s
     9980<br># stopping criteria
     9981<br>stop temperature 3K linear
     9982<br>stop neutral hydrogen column density 18
     9983<br>#
     9984<br># command exercised =========
     9985<br>#
     9986<br>set lya 21cm constant
     9987<br>#
     9988<br># commands controlling output    =========
     9989<br>#
     9990<br>set save prefix "lya-21cm-constant"
     9991<br>save hydrogen 21cm ".21cm" last
     9992<br>save hydrogen lya ".lya" last
     9993<br>save overview ".ovr" last
     9994<br>#
     9995<br>#
     9996<br>#
     9997<br>#
     9998<br>#
     9999<br># # ========================================
     10000</kbd><p>
     10001This is one of the sims employed by Shaw, Ferland, & Hubeny 2017, ApJ, 843, 149.
     10002It exercises the Snu=constant case to column density of 1e18, while the original
     10003paper used a 1e20 stopping criterion.
     10004</p><hr><kbd><h2>lya-21cm-excitation.in</h2>  </kbd><h2><I>test effect of lya pump on spin temperature
     10005</I></h2><kbd><br>title test effect of lya pump on spin temperature
     10006<br>#
     10007<br># commands controlling continuum =========
     10008<br>#
     10009<br>table ism
     10010<br>extinguish column 22
     10011<br>CMB, z=0
     10012<br>#
     10013<br># commands for density & abundances =========
     10014<br># set the density and composition, ism with grains
     10015<br>#
     10016<br>hden 2
     10017<br>abundance ism
     10018<br>#
     10019<br># other commands for details     =========
     10020<br>#
     10021<br># this is an important ionization source
     10022<br>cosmic rays background 
     10023<br># optical depth
     10024<br>double
     10025<br>iterate
     10026<br>turbulence 3 km/s
     10027<br># stopping criteria
     10028<br>stop temperature 3K linear
     10029<br>stop neutral hydrogen column density 18
     10030<br>#
     10031<br># command exercised =========
     10032<br>#
     10033<br>set lya 21cm excitation
     10034<br>#
     10035<br># commands controlling output    =========
     10036<br>#
     10037<br>set save prefix "lya-21cm-excitation"
     10038<br>save hydrogen 21cm ".21cm" last
     10039<br>save hydrogen lya ".lya" last
     10040<br>save overview ".ovr" last
     10041<br>#
     10042<br>#
     10043<br>#
     10044<br>#
     10045<br>#
     10046<br># # ========================================
     10047</kbd><p>
     10048This is one of the sims employed by Shaw, Ferland, & Hubeny 2017, ApJ, 843, 149.
     10049It exercises the Snu~B(Texc) case to column density of 1e18, while the original
     10050paper used a 1e20 stopping criterion.
     10051</p><hr><kbd><h2>lya-21cm-kinetic.in</h2>  </kbd><h2><I>test effect of lya pump on spin temperature
     10052</I></h2><kbd><br>title test effect of lya pump on spin temperature
     10053<br>#
     10054<br># commands controlling continuum =========
     10055<br>#
     10056<br>table ism
     10057<br>extinguish column 22
     10058<br>CMB, z=0
     10059<br>#
     10060<br># commands for density & abundances =========
     10061<br># set the density and composition, ism with grains
     10062<br>#
     10063<br>hden 2
     10064<br>abundance ism
     10065<br>#
     10066<br># other commands for details     =========
     10067<br>#
     10068<br># this is an important ionization source
     10069<br>cosmic rays background 
     10070<br># optical depth
     10071<br>double
     10072<br>iterate
     10073<br>turbulence 3 km/s
     10074<br># stopping criteria
     10075<br>stop temperature 3K linear
     10076<br>stop neutral hydrogen column density 18
     10077<br>#
     10078<br># command exercised =========
     10079<br>#
     10080<br>set lya 21cm kinetic
     10081<br>#
     10082<br># commands controlling output    =========
     10083<br>#
     10084<br>set save prefix "lya-21cm-kinetic"
     10085<br>save hydrogen 21cm ".21cm" last
     10086<br>save hydrogen lya ".lya" last
     10087<br>save overview ".ovr" last
     10088<br>#
     10089<br>#
     10090<br>#
     10091<br>#
     10092<br>#
     10093<br># # ========================================
     10094</kbd><p>
     10095This is one of the sims employed by Shaw, Ferland, & Hubeny 2017, ApJ, 843, 149.
     10096It exercises the Snu~B(Tkin) case to column density of 1e18, while the original
     10097paper used a 1e20 stopping criterion.
    978910098</p><hr><kbd><h2>nlr_lex00.in</h2>  </kbd><h2><I>NLR model for Lexington 2000 Meeting
    979010099</I></h2><kbd><br>title NLR model for Lexington 2000 Meeting
     
    1021610525<br>save lines, array "orion_hii_open.lina" units microns last no hash
    1021710526<br>save line emissivity "orion_hii_open.ems" last no hash emergent
     10527<br>H  1 4861.33A
    1021810528<br>blnd  5199
    1021910529<br>O  1  6300.30
     
    1143611746<br>#
    1143711747</kbd><p>
     11748</p><hr><kbd><h2>pdr_minimal.in</h2>  </kbd><h2><I>test physical conditions at the illuminated face of a PDR
     11749</I></h2><kbd><br>title test physical conditions at the illuminated face of a PDR
     11750<br>#
     11751<br># commands controlling continuum =========
     11752<br>table draine 50000
     11753<br>extinguish 24
     11754<br>#
     11755<br># commands for density & abundances =========
     11756<br>hden 5.5
     11757<br>element helium abundance -1.00 
     11758<br>element lithium     off 
     11759<br>element beryllium   off
     11760<br>element boron       off
     11761<br>element carbon      off
     11762<br>element oxygen      off
     11763<br>element fluorine    off
     11764<br>element neon        off 
     11765<br>element sodium      off 
     11766<br>element magnesium   off 
     11767<br>element aluminum    off 
     11768<br>element silicon     off
     11769<br>element phosphorus  off
     11770<br>element sulphur     off
     11771<br>element chlorine    off 
     11772<br>element argon       off 
     11773<br>element potassium   off
     11774<br>element calcium     off
     11775<br>element scandium    off 
     11776<br>element titanium    off 
     11777<br>element vanadium    off 
     11778<br>element chromium    off 
     11779<br>element manganese   off 
     11780<br>element iron        off
     11781<br>element cobalt      off
     11782<br>element nickel      off 
     11783<br>element copper      off 
     11784<br>element zinc        off
     11785<br>#
     11786<br># other commands for details     =========
     11787<br>constant temperature 50 linear
     11788<br>set dr 1
     11789<br>stop zone 2
     11790<br>stop temperature off
     11791<br>#
     11792<br># commands controlling output    =========
     11793<br>set save prefix "pdr_minimal"
     11794<br>save performance ".per" last
     11795<br>save overview ".ovr" last
     11796<br>save molecules ".mol" last
     11797<br>save leiden ".lei" last
     11798<br>save leiden lines ".lin" last
     11799<br>#
     11800<br>#
     11801<br># IF EITHER OF THESE MONITORS NEEDS TO BE ADJUSTED, CHECK THAT THE IONIZATION
     11802<br># CONDITIONS IN ZONE 1 AND 2 ARE IN VERY GOOD AGREEMENT!
     11803<br>#
     11804<br># pdr_minimal.in
     11805<br># class pdr
     11806<br># ========================================
     11807</kbd><p>
     11808This model is derived from the F4 model from the Leiden workshop (Roellig et
     11809al. 2007, A&A, 467, 187). It has been reduced to a two-zone model in order to
     11810test the ionization conditions at the face of the PDR. Older versions of the
     11811code had a bug where the ionization in zone 1 was many dex lower than in zone
     118122. The conditions in zone 1 were wrong and should have been similar to the
     11813conditions in zone 2. Here we test that the code doesn't regress. See also
     11814ticket #358: https://wiki.nublado.org/ticket/358
     11815<p>
     11816The ionization in this sim is produced by continuum pumping of the metastable
     11817levels of N I, followed by photoionization out of the metastable levels of N I.
     11818See Ferland et al., 2012, ApJ, 757, 79. So this pumping and ionization mechanism
     11819is also tested by this sim.
    1143811820</p><hr><kbd><h2>pdr_orion_veil.in</h2>  </kbd><h2><I>Orion's veil
    1143911821</I></h2><kbd><br>title Orion's veil
     
    1391714299<br>#
    1391814300<br># commands controlling output    =========
    13919 <br>normalize to "O  8" 18.9709A
     14301<br>normalize to "O  8" 18.9689A
    1392014302<br>print line faint -3 log
    1392114303<br>print line cumulative
  • branches/c17_branch/tsuite/auto/doc_tsuite.txt

    r11780 r14395  
    7474func\_sdrmin & test set drmin command \\
    7575func\_set\_ion & test impact of setting ionization  \\
     76func\_stopcol & test stop column density "species" command \\
    7677func\_stopline1 & test stop line command \\
    7778func\_stopline2 & test stop line command \\
     
    8586func\_testmole & this runs the standard, one command, test, which contains many asserts \\
    8687func\_tlaw & test model with tlaw table \\
     88func\_trans\_lumi & test transmitted continuum in luminosity mode \\
    8789func\_trans\_read & second of func\_trans\_save/func\_trans\_read pair, use transmitted continuum \\
     90func\_trans\_read\_lumi\_scale & test read transmitted continuum in luminosity mode \\
    8891func\_trans\_read\_scale & second of func\_trans\_save/func\_trans\_readread pair \\
    8992func\_trans\_save & first of func\_trans\_save/func\_trans\_read pair, save continuum \\
     93func\_trans\_save\_lumi & test save transmitted continuum in luminosity mode \\
    9094grains\_hot & test temperature of gas and dust in high energy density environment \\
    9195grains\_hot\_wd01 & test temperature of gas and dust in high energy density environment \\
     
    214218limit\_vbhum & compare with Van Blerkom and Hummer exact RT results \\
    215219limit\_veryveryfast & very fast simulation for Purify/valgrind \\
     220lya-21cm-constant & test effect of lya pump on spin temperature \\
     221lya-21cm-excitation & test effect of lya pump on spin temperature \\
     222lya-21cm-kinetic & test effect of lya pump on spin temperature \\
    216223nlr\_lex00 & NLR model for Lexington 2000 Meeting \\
    217224nlr\_liner & NLR liner model \\
     
    246253pdr\_leiden\_v3 & Leiden meeting model 7 \\
    247254pdr\_leiden\_v4 & Leiden meeting model 8 \\
     255pdr\_minimal & test physical conditions at the illuminated face of a PDR \\
    248256pdr\_orion\_veil & Orion's veil \\
    249257pdr\_th85ism & TH85 PDR with ISM grains \\
  • branches/c17_branch/tsuite/slow/doc_tsuite.htm

    r11780 r14395  
    433433<br>element berylium off
    434434<br>element boron off
     435<br>element limit -7 off
    435436<br>cosmic rays background linear 0.1266
    436437<br>cmb
     
    538539<br>init file="ism.ini"
    539540<br>Abundances H II region no grains                                               
    540 <br>grains orion                                                                    
     541<br>grains orion no qheat
    541542<br># these were actually used in the paper
    542 <br>grains PAH
     543<br>grains PAH no qheat
    543544<br>#
    544545<br># commands controlling geometry  =========
     
    13521353<br>hden 5.88e-2 linear
    13531354<br>constant pressure reset
     1355<br># >> chng 20 oct 05, from -6 to -5 for load balancing
     1356<br>element limit off  -5
    13541357<br>#
    13551358<br># commands controlling geometry  =========
     
    13951398<br>hden 5.88e-2 linear
    13961399<br>constant pressure reset
     1400<br># >> chng 20 oct 05, from -6 to -5 for load balancing
     1401<br>element limit off  -5
    13971402<br>#
    13981403<br># commands controlling geometry  =========
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