The OI844.6 nm emission in evening twilight
Author:
Publisher
American Geophysical Union (AGU)
Subject
General Earth and Planetary Sciences,Geophysics
Link
http://www.agu.org/journals/gl/v016/i012/GL016i012p01449/GL016i012p01449.pdf
Reference18 articles.
1. OI (7774Å) and OI (8446Å) emission in aurora;Christensen;J. Geophys.Res.,1978
2. Rotational analysis of hydroxyl vibration-rotation emission bands: Molecular constants for OH X2Π, 6 ≤ υ ≤ 10;Coxon;Can. J. Phys.,1982
3. Observations of the optical spectrum of the dayside magnetospheric cleft aurora;Gault;Planet. Space Sci.,1981
4. PRESTO:a programmable etalon spectrometer for twilight observations;Gault;Appl. Opt.,1983
5. A study of the auroral OI feature at 8446Å;Harang;Planet. Space Sci.,1962
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1. Global‐Scale Observations and Modeling of Far‐Ultraviolet Airglow During Twilight;Journal of Geophysical Research: Space Physics;2020-03
2. Evidence for Radiative Recombination of O+ Ions as a Significant Source of O 844.6 nm Emission Excitation;Journal of Geophysical Research: Space Physics;2018-04
3. A study of OI 844.6nm dayglow emission under geomagnetic storm conditions;Advances in Space Research;2015-06
4. Morphology of OI 8446Å dayglow emission;Advances in Space Research;2010-07
5. Photoelectron impact excitation of OI 8446 Å emission observed from Arecibo Observatory;Journal of Geophysical Research: Space Physics;2008-01
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