| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 8140965 | Journal of Atmospheric and Solar-Terrestrial Physics | 2012 | 5 Pages |
Abstract
⺠We studied the behavior of the OI 630 and 557.7 nm nightglow during magnetic storms. ⺠The OI 630 and 557.7 nm emissions were similar in shape and synchronous. ⺠At the same time these two emissions were correlated with the TEC. ⺠The 557.7 nm disturbances may result from the O2+ dissociative recombination. ⺠The ratio of V557.7/V630 may vary during magnetic storms at mid-latitudes.
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Physical Sciences and Engineering
Earth and Planetary Sciences
Geophysics
Authors
L.Ð. Leonovich, A.V. Mikhalev, V.A. Leonovich,