First direct optical observations of plasma flows using afterglow of O in discrete aurora

Details First direct optical observations of plasma flows using afterglow of O in discrete aurora First direct optical observations of plasma flows using afterglow of O in discrete aurora

Feb 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jastp..71..228d&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 71, Issue 2, p. 228-238.

Physics

1

Ionosphere, Plasma Drift, Aurora, Oxygen Ion, Electric Fields

Scientific paper

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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