A program to calculate coronal emission line strengths
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https://elsevier.digitalcommonsdata.com/datasets/jn92dgc27p
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资源简介：
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)
创建时间：
2019-11-11
