First direct optical observations of plasma flows using afterglow of O + in discrete aurora
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...
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Published in | Journal of atmospheric and solar-terrestrial physics Vol. 71; no. 2; pp. 228 - 238 |
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Main Authors | , , , , , , |
Format | Journal Article |
Language | English |
Published |
Kidlington
Elsevier Ltd
01.02.2009
Elsevier |
Subjects | |
Online Access | Get full text |
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Summary: | 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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ISSN: | 1364-6826 1879-1824 1879-1824 |
DOI: | 10.1016/j.jastp.2008.11.015 |