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The effects of solar flares, coronal mass ejections, and co-rotating interaction regions on the Venusian 5577 A oxygen green line
Bibcode: 2015PhDT........68G
Gray, Candace
The Venusian 5577.3 A OI (1S - 1D) (oxygen green line) nightglow emission is known to be highly temporally variable. The reason for this variability is unknown. We propose that the emission is due to electron precipitation from intense solar storms. For my dissertation, I observed the Venusian green line after solar flares, coronal mass ejections …
2015
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Ph.D. Thesis
VenusExpress
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