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Optical flow analysis of the aurora borealis
KTH, School of Electrical Engineering (EES), Space and Plasma Physics.ORCID iD: 0000-0003-2422-5426
2006 (English)In: IEEE Geoscience and Remote Sensing Letters, ISSN 1545-598X, E-ISSN 1558-0571, Vol. 3, no 1, 159-163 p.Article in journal (Refereed) Published
Abstract [en]

Optical observations of the aurora have traditionally focused on the structure, intensity, and wavelength of the emissions. But the apparent motion of auroral forms offers another important diagnostic tool for investigating this poorly understood phenomenon. Prior analyses of auroral motion have focused on tracing individual features. In this letter, we investigate the feasibility of deriving the entire two-dimensional velocity field automatically using robust optical flow estimation. The analysis is applied to two narrow-field video sequences. Both examples are rich in small-scale structure and motion, but appear very different to the eye. The robust optical flow estimator performed well for regions of dense turbulent motion, while sheared flow and flow which is perpendicular to image intensity gradients, was poorly resolved. The relative magnitude of the outliers provides a quantitative measure of the validity of the underlying flow model and, hence, a means of automatically differentiating among auroral forms with differing physical origins. The technique can be used to deduce ionospheric electric fields and neutral winds, and the flow fields yield important physical information about the generation mechanism.

Place, publisher, year, edition, pages
2006. Vol. 3, no 1, 159-163 p.
Keyword [en]
aurora borealis, optical flow, robust statistics, acceleration, arcs
URN: urn:nbn:se:kth:diva-15388DOI: 10.1109/lgrs.2005.860981ISI: 000234898700034ScopusID: 2-s2.0-31144456479OAI: diva2:333429
QC 20100525Available from: 2010-08-05 Created: 2010-08-05Bibliographically approved

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Ivchenko, Nickolay V.
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