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Messages 423 - 453 of 517   Oldest  |  < Older  |  Newer >  |  Newest
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423
Thanks, Rob. I've recreated the problem here, and it appears in our development version as well. I'll let you know when I've found a fix. There is clearly ...
rporter@...
ryan_l_porter
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Mar 1, 2008
7:34 pm
424
We are looking at ionization fractions in primordial gas at low densities (n_H ~ 1e-5 but that isn't very important) with effectively no radiation background....
James
james_wadsley
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Mar 4, 2008
7:30 pm
425
... i got identical ionizations with and without charge transfer for a primordial cloud irradiated by a STE blackbody at 12,000K. please post an example of...
gary_ferland
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Mar 4, 2008
9:12 pm
426
... We have effectively no radiation background so the ionization is primarily collisional and we fix the temperature at the given value. We find this result...
James
james_wadsley
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Mar 5, 2008
5:01 pm
427
... effectively ... the code includes a large chemistry network. the reactions that are responsible for the He ionization are described in Lepp et al. J Phys ...
gary_ferland
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Mar 7, 2008
5:44 pm
428
I am running a grid of models with the new Kurucz models and a range of ionizing fluxes: hden 4 abundances _ism punch continuum "k350c.con" units microns ...
rdblum5
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Mar 14, 2008
10:41 pm
429
Good Day, all, I think I've come across something that Cloudy allows the user to do, but perhaps shouldn't (?): the "punch lines emissivity" allows one to...
John Everett
everett@...
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Mar 15, 2008
5:16 pm
430
Hi, The only thing you can do here is write your own routine GrnVryDpth(). A stub is located at the end of the file grains.cpp. With this you can define a...
Peter van Hoof
peter_van_hoof
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Mar 15, 2008
7:37 pm
431
Hi, I was wondering how high a priority this is. Quite a few of my numbers are off when using the grid command. If its not very high on the todo list, then...
Rob Wiersma
wiersmarp
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Mar 17, 2008
9:21 am
432
Hi Rob, This is a long standing problem in the code. Optimizer runs suffer from the same problem. After each model the code needs to be returned to exactly the...
Peter van Hoof
peter_van_hoof
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Mar 17, 2008
1:19 pm
433
Hi Rob, It looks like the solution is a simple change in parse_interp.cpp. At line 415, the source should be changed from this for( i=npairs; i <...
Ryan Porter
ryan_l_porter
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Mar 17, 2008
1:26 pm
434
Thanks Peter. I will give it a try. -bob ... GrnVryDpth(). A ... define a ... The ... clear. ... abundance...
rdblum5
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Mar 18, 2008
5:11 pm
435
You might consider bringing the grain material out into the gas phase when they reach the sublimation point. There are options to vary the gas-phase abundance...
gary_ferland
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Mar 18, 2008
5:20 pm
436
Hi there, this message had been moved into my spam folder - sorry for missing it. You could do a clumped medium - but clumps don't form in a 1D outflow. You...
gary_ferland
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Mar 18, 2008
5:27 pm
437
... Dear Gary, Thanks for the reference. The Lepp et al. and Stancil et al. papers refer extensively to H+ + He -> HeH+ but do not explicitly list associated...
James
james_wadsley
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Mar 19, 2008
7:16 pm
438
Hi James, thanks for the persistence! it is a bug. There is a recombination rate that was entered into the wrong array as an ionization process. The fix is...
gary_ferland
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Mar 22, 2008
5:51 pm
439
the bug fix had a bug - after the correction the source will read as if( phycon.te > 6000. ) atmdat.HCharExcRecTo[ipHELIUM][0] +=...
gary_ferland
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Mar 22, 2008
7:14 pm
440
... 15*pow(phycon.te/1e4,2.06)* ... Hi All, The previous version of the source with (...ExcIonOf) looked like the fit for the reverse reaction which appears in...
phillipstancil
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Mar 23, 2008
10:58 pm
441
Hi, I have a simulation "!The model has modest optical depth to electron scattering; tau=0.25". I want to know if the total optical depth in the mtable...
bassemsabra
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Mar 25, 2008
8:46 am
442
Hi Ryan, Looks good, thanks a lot! Rob ... At line ... tested ... 0. All ... point to ... o=-30.0 ... v=-30.0 ... 40102 ... o=-30.0 ... v=-30.0...
Rob Wiersma
wiersmarp
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Mar 25, 2008
2:53 pm
443
Hi there, Interesting point. The basic problem is, as you say, that the attenuated incident continuum is part of the quantity that goes into the continuum...
gary_ferland
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Mar 25, 2008
9:57 pm
444
I used version 07.02.01 (and 07.02.00) of Cloudy with the input given below and the program stopped because of a floating point exception. If I remove either...
kilian.braun
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Mar 26, 2008
11:38 am
445
Hi Kilian, Thanks for bringing this to our attention! I have been able to reproduce the problem. The fix is quite straightforward. In Cloudy 07.02.01 take the...
Peter van Hoof
peter_van_hoof
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Mar 26, 2008
4:36 pm
446
... Hi there, line and continuum optical depths are kept separate. Line optical depths scatter the photon within the line and excite the upper level. Coherent...
gary_ferland
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Mar 30, 2008
2:03 am
447
Hi there, I've been playing around with the 'No Induced Processes' command. I've uploaded a plot showing cooling vs. temperature, and it shows that there is an...
Rob Wiersma
wiersmarp
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Mar 31, 2008
3:22 pm
449
Hi there, that command does many things, but most likely the process affecting what you are doing is UTA ionization. try replacing the "no induced" with "no...
gary_ferland
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Mar 31, 2008
4:58 pm
450
Hi Gary, I'd vote for keeping the output of continuum-band emissivity (without the transmitted continuum component). For my particular application (modelling...
John Everett
everett@...
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Apr 1, 2008
5:00 pm
451
Hi, I am trying to make heating and cooling rates grid with different temperatures(T), densities, metallicities and redshifts, using a modified code from...
kawata_daisuke
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Apr 4, 2008
3:57 am
452
Hi, This is a known problem that will be fixed in the next release. The program runs out of file descriptors. If you include the statement: fclose( ioFILE ); ...
Peter van Hoof
peter_van_hoof
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Apr 4, 2008
5:00 pm
453
Thanks a lot, Peter, for your prompt and nice sugestion! It works beautifully after the change, and now I can make a big grid. Thanks a lot again. Daisuke ... ...
kawata_daisuke
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Apr 4, 2008
10:59 pm
Messages 423 - 453 of 517   Oldest  |  < Older  |  Newer >  |  Newest
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