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Messages 410 - 439 of 486   Oldest  |  < Older  |  Newer >  |  Newest
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410
Hello, When a run a cloudy simulation, I use as an input a ionizing continuum given by the SED of an evolutionary synthesis code.This SED contains the sum...
mariluzmartin
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Feb 19, 2008
2:15 pm
411
... This depends on what is calculated by the synthesis code. I assume this is an average interstellar radiation field comprised of the emissions of nearby...
peter_van_hoof
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Feb 19, 2008
3:25 pm
412
Hi, I'm getting the following crash when trying to run cloudy to compute cooling and heating rates at a fixed temperature (10^4K): PROBLEM DISASTER An assert...
kiniandr
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Feb 20, 2008
8:18 pm
413
Hi Andrew, Thanks for lettings us know. I'll look into and get back to you shortly. Cheers, Ryan ... Ryan L. Porter, Post-doctoral Scholar Visiting: ...
Ryan Porter
ryan_l_porter
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Feb 21, 2008
1:54 am
414
Hi Andrew, We have so far not been able to reproduce this problem. Can you give us the precise compiler options you used to compile the code and also the Linux...
peter_van_hoof
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Feb 21, 2008
2:21 pm
415
Hi Andrew, Another question. Did you run the test suite with your executable and were there any problems? Cheers, Peter....
peter_van_hoof
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Feb 21, 2008
2:32 pm
416
Hi Peter, ... Thanks for looking in to this. Here's the relevant information: Linux distribution: Fedora 8 gcc version: gcc version 4.1.2 20070925 (Red Hat...
kiniandr
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Feb 21, 2008
5:01 pm
417
... This error is occuring when I run cloudy as a subroutine from a driver program. If I run cloudy directly and feed in the same commands I get no error. So,...
kiniandr
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Feb 21, 2008
5:31 pm
418
... Even with this setup I cannot reproduce the problem, but then I am using a standard release version of g++ 4.1.2... Try changing the compiler options to ...
Peter van Hoof
peter_van_hoof
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Feb 21, 2008
6:05 pm
419
... optimizations ... bug... That doesn't seem to fix the problem unfortunately. I'm reasonably convinced that there's some issue with my driver program -...
kiniandr
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Feb 21, 2008
6:31 pm
420
... You could try running the program through valgrind, should only take a couple of minutes. It catches a lot of bugs: valgrind cloudy.exe > /dev/null Peter....
Peter van Hoof
peter_van_hoof
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Feb 21, 2008
6:35 pm
421
Hi, I was wondering if it is possible to model an outflowing clumped gas using Cloudy? I have been using Cloudy to model clumped gas using the filling factor...
Andrea Ruff
a_ruff
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Feb 25, 2008
12:38 am
422
For some reason the following gives me a thrown assert: hden 0.0 vary grid range from -8 to 0 with 8 dex steps interpolate (-9.00000 -30.000) (-3.10302...
Rob Wiersma
wiersmarp
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Feb 28, 2008
2:32 pm
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
Messages 410 - 439 of 486   Oldest  |  < Older  |  Newer >  |  Newest
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