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Intensity variations in the solar extreme ultraviolet spectrum observed by OSO-I

Published online by Cambridge University Press:  14 August 2015

Werner M. Neupert
Werner M. Neupert*
Affiliation:
Goddard Space Flight Center, Greenbelt, Maryland U.S.A.

Abstract

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This paper reviews solar extreme ultraviolet observations made in the spectral region λ170 — λ400 by the first Orbiting Solar Observatory during March, April, and May, 1962. Application of the data to the identification of emission lines in this spectral region is discussed. The observations are compared with concurrent 2800 MHz radio emission and other measurements of solar activity.

On passe en revue les observations de l'extrême ultraviolet solaire obtenues en mars, avril et mai 1962 par le satellite OSO. On discute l'emploi de ces résultats pour l'identification des raies d'émission dans le domaine spectral 170-400 Å. Ces observations sont comparées à celles du flux radioélectrique sur 2800 MHz et à d'autres mesures de l'activité solaire.

Резюме

Резюме

Просматрены наблюдения в крайней ультрафиолетовой солнечной области, полученные в марте, апреле и мае 1962г спутником OSO. Обсуждено применение этих результатов для отождествления эмиссионных линий в спектральной области 170-400 Å. Эти наблюдения сравнены с наблюдениями радиоэлектрического потока в 2800 Мгц и с другими измерениями солнечной активности.

Type
Session I. Far Ultra-Violet Radiation : The Sun
Information
Symposium - International Astronomical Union , Volume 23: Astronomical Observations from Space Vehicles , 1965 , pp. 31 - 41
Copyright
Copyright © CNRS 1965 

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