A program to calculate coronal emission line strengths

Published: 1 January 1977| Version 1 | DOI: 10.17632/jn92dgc27p.1
P.L. Dufton


Title of program: AATWAB Catalogue Id: ACXE_v1_0 Nature of problem This computer program is used to calculate the intensities of emission spectral lines from the upper solar atmosphere. The optically thin approximation is used and the validity of this assumption is checked by calculating line centre optical depths. Account may be taken of collisional transitions (by electron and proton impact) and spontaneous radiative transitions between all the selected levels of the chosen ion in calculating the intensities. The program integrates these intensities through w ... Versions of this program held in the CPC repository in Mendeley Data ACXE_v1_0; AATWAB; 10.1016/0010-4655(77)90024-8 This program has been imported from the CPC Program Library held at Queen's University Belfast (1969-2019)



Astronomy, Astrophysics, Computational Physics, Plasma Physics