Published March 1975 | Version v1
Journal article Metadata-only

The excitation of several iron and calcium lines in the visible spectrum of the solar corona

Creators

  • 1. University Coll., London (UK). Dept. of Physics

Description

New atomic data have been obtained for the coronal ions Fe X, Fe XI, Fe XIV, Ca XII, Ca XIII and Ca XV, using a computer package developed at University College, London. Energy levels and radiative transition probabilities have been computed allowing for configuration interaction and relativistic effects. The electron scattering problem has been solved using the 'distorted wave' approach.

Additional details

Identifiers

DOI
10.1093/mnras/170.3.651;

Publishing Information

Journal Title
Monthly Notices of the Royal Astronomical Society
Journal Volume
170
Journal Issue
3
Series
Mon. Not. R. Astron. Soc.
Journal Page Range
651-689
ISSN
0035-8711

INIS

Country of Publication
United Kingdom
Country of Input or Organization
United Kingdom
INIS RN
6188935
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
ATOMIC MODELS; CALCIUM IONS; CONFIGURATION INTERACTION; DISTORTED WAVE THEORY; ELECTRONIC STRUCTURE; ELECTRONS; ENERGY LEVELS; EXCITATION; IRON IONS; RELATIVITY THEORY; SCATTERING; SOLAR CORONA; SPECTRA; VISIBLE RADIATION
Descriptors DEC
CHARGED PARTICLES; ELECTROMAGNETIC RADIATION; ELEMENTARY PARTICLES; ENERGY-LEVEL TRANSITIONS; FERMIONS; FIELD THEORIES; GENERAL RELATIVITY THEORY; IONS; LEPTONS; MATHEMATICAL MODELS; RADIATIONS

Optional Information

Notes
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