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 |
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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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