The Extreme-Ultraviolet Spectrum of a Solar Active Region

The Extreme-Ultraviolet Spectrum of a Solar Active Region

Extreme-ultraviolet spectra (280-1370 A) of the brightest point in McMath Region 10266 and of the quiet solar atmosphere are presented as measured by the Harvard scanning spectrometer on OSO-6. Line identifications and physical parameters of the active region are discussed. (auth)

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Bibliographische Detailangaben
Veröffentlicht in:Astrophys. J., v. 182, no. 1, pp. 321-333 v. 182, no. 1, pp. 321-333, 1973-05, Vol.182, p.321
Hauptverfasser: Dupree, A. K., Huher, M. C. E., Noyes, R. W., Parkinson, W. H., Reeves, E. M., Withbroe, G. L.
Format: Artikel
Sprache:eng
Schlagworte:
CHEMICAL COMPOSITION
EMISSION SPECTRA
LINE WIDTHS
N56400 -Physics (Astrophysics & Cosmology)-Solar Phenomena
SOLAR ACTIVITY- ULTRAVIOLET SPECTRA
SUN
SUNSPOTS- ULTRAVIOLET SPECTRA
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Zusammenfassung:Extreme-ultraviolet spectra (280-1370 A) of the brightest point in McMath Region 10266 and of the quiet solar atmosphere are presented as measured by the Harvard scanning spectrometer on OSO-6. Line identifications and physical parameters of the active region are discussed. (auth)
ISSN:0004-637X
1538-4357
DOI:10.1086/152139