Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
1777320 | Journal of Atmospheric and Solar-Terrestrial Physics | 2009 | 11 Pages |
Abstract
Imaging of active structured aurora in the forbidden O+ ion line at 732.0 nm provides a possibility of direct observation of plasma drifts in the topside ionosphere. The metastable O+ 2P state has a radiative lifetime of 5 s, so the oxygen ions can be detected after the precipitation creating them has ceased. The decay time of the O+ emission is studied and modelled with a time-dependent electron transport and ion chemistry model. Four examples are given of O+ afterglow observed with the multi-spectral imager, auroral structure and kinetics (ASK), which was located near Tromsø, Norway, in 2006. Estimates are given of drift velocities resulting from the analysis of the afterglow motions. Bulk plasma velocities of 340 and 720 m/s directed eastwards were found for two afterglowing arc filaments, corresponding to southward electric fields of 18 and 40 mV/m, respectively.
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Authors
H. Dahlgren, N. Ivchenko, B.S. Lanchester, M. Ashrafi, D. Whiter, G. Marklund, J. Sullivan,