wiki:ContributedMaterial

Version 7 (modified by Gary J. Ferland, 4 weeks ago) (diff)

WARPFIELD links

Contributed material


Morisset created pyCloudy. This allows you to

  • Define and write input file(s) for Cloudy code. As you can have it in a code, you may generate automatically sets of input files, changing parameters from one to the other.
  • Read the Cloudy output files and play with the data: you will be able to plot line emissivity ratio vs. the radius of the nebula, the electron temperature, or any Cloudy output.
  • Build pseudo-3D models, a la Cloudy_3D. This means: run a set of models, changing parameters (e.g. inner radius, density) following angular laws, read the outputs of the set of models and interpolate the results (Te, ne, line emissivities) in a 3D cube.

They have a discussion forum to answer questions.

Morisset and Stasinska created Cloudy 3D. This uses IDL scripts to drive Cloudy as a subprogram and create simulations of complex geometries.


WARPFIELD solves the acceleration against gravity accounting for feedback from winds, radiation, and SNe. More information is here and a paper describing it is here.

Wang Ye's helper scripts for extracting information related to the gas cooling are given here.

Kyujin Kwak's grids of radiation fields from turbulent mixing layer simulations, suitable for use in the interpolate command, are here.


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Attachments (2)

  • totl2blnd (1.2 KB) - added by mchatzikos 4 years ago. Perl script searches all input files (*.in) for a monitor command at the requested wavelength, and replaces the keyword 'totl' with 'blnd'.
  • totl2blnd.2 (1.2 KB) - added by mchatzikos 4 years ago. Perl script searches all input files (*.in) for a monitor command at the requested wavelength, and replaces the keyword 'totl' with 'blnd'.

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