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Identifications of Emission Lines in the EUV Solar Spectrum

Published online by Cambridge University Press:  12 April 2016

Carole Jordan
Carole Jordan*
Affiliation:
Astrophysics Research Unit, Culham Laboratory, Abingdon, Berks., England

Extract

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In this brief review of solar line identifications the progress made since the previous conference in this series, which was held in Maryland in 1968, will be discussed.

Only lines which appear in emission when seen in the solar disk will be included, thus excluding lines from low stages of ionization at wavelengths of above about 2000Å which can appear in emission at the limb.

It is convenient to divide the solar spectrum between about 1.5 Å and 2300 Å into wavelength regions, since the various types of transitions which will be discussed tend to appear over restricted wavelength ranges.

Type
Section III / Stellar and Solar UV Radiation
Information
International Astronomical Union Colloquium , Volume 14: Special Issue: Ultraviolet and X-Ray Spectroscopy of Astrophysical and Laboratory Plasmas , November 1972 , pp. 595 - 605
Copyright
Copyright © Reidel 1972

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