Is the O2(a1Δg) Venus nightglow emission controlled by solar activity?
DOI: 10.1016/j.icarus.2015.08.030
Bibcode: 2015Icar..262..170S
Gérard, Jean-Claude; Soret, Lauriane
Belgium
Abstract
Several past studies showed that the O2(a1Δg) Venus nightglow emission at 1.27 μm is highly variable on a timescale of hours. We examine whether the intensity of this emission shows a more global trend linked to solar activity.
2015
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Icarus
VenusExpress
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