SKYLAB observations of the solar O I resonance triplet

Details SKYLAB observations of the solar O I resonance triplet SKYLAB observations of the solar O I resonance triplet

Dec 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985a%26a...153..116r&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 153, no. 1, Dec. 1985, p. 116-124.

Astronomy and Astrophysics

Astrophysics

7

Chromosphere, Oxygen Spectra, Resonance Lines, Solar Spectra, Ultraviolet Spectra, Atomic Energy Levels, Line Spectra, Skylab Program, Solar Limb

Scientific paper

Profile variations from center to limb, as well as at different heights above the quiet solar limb, are illustrated by profile observations of the solar O I resonant triplet at 1302, 1304, and 1306 A that were obtained with the Skylab S082-B spectrograph. Since these lines share a common upper energy level, source function equality should exist for them when the lower states are populated according to their statistical weights. Profile congruency and profile inversion calculations comparisons show, however, that this is not the case, suggesting either errors in the fine structure collision rates, or the H I Ly-beta flux preferentially depopulating the 1302 A lower level, or two-dimensional transfer effects.

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