Computation of line and continuum radiation from thermal radioastronomical sources

Published: 1 January 1975| Version 1 | DOI: 10.17632/wmy9pnpg8r.1
M. Brocklehurst, M. Salem


Abstract Title of program: RCMBLN Catalogue number: AAEG Program obtainable from: CPC Program Library, Queen's University of Belfast, N. Ireland (see application form in this issue). Computer: IBM 360/65; Installation: University College London Computer Centre. Operating system: OS Programming language used: FORTRAN IV High speed storage required: 25000 words No. of bits in a word: 32 Overlay structure: None No. of magnetic tapes required: 2 (optional) Other peripherals used: Card reader, line printer... Title of program: SELECT BN,CN VALUES Catalogue Id: AAEH_v1_0 Nature of problem The departure coefficients from thermodynamic equilibrium, bn, and their derivatives, cn, are required for the computation of intensities and profiles of hydrogen recombination lines from thermal radioastronomical sources. These coefficients have been computed by Brocklehurst(1970) for values of n up to 300, for 6 values of electron temperature, and for 8 values of electron density. As it is not expected that intensity calculations will be required for more than a few lines at a time, and as the ... Versions of this program held in the CPC repository in Mendeley Data aaeh_v1_0; SELECT BN,CN VALUES; 10.1016/0010-4655(75)90012-0 This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)



Astronomy, Astrophysics, Computational Physics