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CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra

Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., Verner, E. M.·1998·Publications of the Astronomical Society of the Pacific

Abstract

ABSTRACT CLOUDY is a large‐scale spectral synthesis code designed to simulate fully physical conditions within an astronomical plasma and then predict the emitted spectrum. Here we describe version 90 (C90) of the code, paying particular attention to changes in the atomic database and numerical methods that have affected predictions since the last publicly available version, C84. The computational methods and uncertainties are outlined together with the direction future development will take. The code is freely available and is widely used in the analysis and interpretation of emission‐line spectra. Web access to the Fortran source for CLOUDY, its documentation Hazy, and an independent electronic form of the atomic database is also described.

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Metadata

Authors
Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., & Verner, E. M.
Venue
Publications of the Astronomical Society of the Pacific
Published
1998-07
Volume
110
Issue
749
Pages
761-778
ISSN
  • 0004-6280 (ISSN-L)
  • 1538-3873
OpenAlex
W2068928940
Cited by
2,494
References
0
FWCI
21.97
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra. https://app.cochat.ai/papers/10.1086/316190
The paper
Ferland, G. J., Korista, K. T., Verner, D. A., Ferguson, J. W., Kingdon, J. B., & Verner, E. M. (1998). CLOUDY 90: Numerical Simulation of Plasmas and Their Spectra. Publications of the Astronomical Society of the Pacific. https://doi.org/10.1086/316190

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