Preliminary results from the Orbiting Solar Observatory 8 - Observations of optically thin lines

Measurements of the C IV and Si IV solar resonance lines have been analyzed to yield mean profiles, a comparison of cell and network profiles, and the behavior of the lines at the extreme solar limb. (AIP)

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Veröffentlicht in:Astrophys. J., Lett.; (United States) Lett.; (United States), 1976-12, Vol.210, p.L107
Hauptverfasser: Shine, R. A., Roussel-Dupre, D., Bruner, E. C., Jr, Chipman, E. G., Lites, B. W., Rottman, G. J., Athay, R. G., White, O. R.
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container_end_page
container_issue
container_start_page L107
container_title Astrophys. J., Lett.; (United States)
container_volume 210
creator Shine, R. A.
Roussel-Dupre, D.
Bruner, E. C., Jr
Chipman, E. G.
Lites, B. W.
Rottman, G. J.
Athay, R. G.
White, O. R.
description Measurements of the C IV and Si IV solar resonance lines have been analyzed to yield mean profiles, a comparison of cell and network profiles, and the behavior of the lines at the extreme solar limb. (AIP)
doi_str_mv 10.1086/182314
format Article
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subjects 640104 - Astrophysics & Cosmology- Solar Phenomena
ATMOSPHERES
ATOMIC IONS
CARBON IONS
CHARGED PARTICLES
CHROMOSPHERE
CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS
ENERGY SPECTRA
FUNCTIONS
GAUSS FUNCTION
IONS
LINE WIDTHS
SILICON IONS
SOLAR ATMOSPHERE
SOLAR CORONA
SPECTRA
title Preliminary results from the Orbiting Solar Observatory 8 - Observations of optically thin lines
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