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The Zeta/solar lines between 170 Å and 220 Å

Published online by Cambridge University Press:  14 August 2015

R. Wilson
R. Wilson*
Affiliation:
Culham Laboratory, Nr. Abingdon, Berkshire, United Kingdom

Abstract

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An important problem in solar physics is the identification of the intense system of spectral lines lying between 170 Å and 220 Å. These lines have also been observed in the high temperature plasma, Zeta, and also in a number of other sources. These sources are reviewed and the experimental evidence relating to the problem of identification is discussed.

L'identification du système de raies intenses entre 170 et 220 Å est un problème important de physique solaire. Ces raies ont aussi été observées dans les plasmas à haute température, la machine Zéta et d'autres sources. Ces résultats sont passés en revue et les données permettant d'aboutir à une identification sont discutées.

Резюме

Резюме

Отождествление системы интенсивных линий между 170 и 220 Å является важной проблемой солнечной физики. Эти линии были также наблюдены в плазмах с высокой температурой, машине Зета и других источниках. Эти результаты просмотрены а данные позволяющие привести к отождествлению обсуждены.

Type
Session III. Interpretation of the Solar X. U. V. Observations
Information
Symposium - International Astronomical Union , Volume 23: Astronomical Observations from Space Vehicles , 1965 , pp. 101 - 103
Copyright
Copyright © CNRS 1965 

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