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Stare Velocities: the Importance of Off-orthogonality and Ion Motions : Volume 21, Issue 3 (30/11/-0001)

By Uspensky, M.

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Book Id: WPLBN0004001275
Format Type: PDF Article :
File Size: Pages 15
Reproduction Date: 2015

Title: Stare Velocities: the Importance of Off-orthogonality and Ion Motions : Volume 21, Issue 3 (30/11/-0001)  
Author: Uspensky, M.
Volume: Vol. 21, Issue 3
Language: English
Subject: Science, Annales, Geophysicae
Collections: Periodicals: Journal and Magazine Collection (Contemporary), Copernicus GmbH
Historic
Publication Date:
-0001
Publisher: Copernicus Gmbh, Göttingen, Germany
Member Page: Copernicus Publications

Citation

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Nozawa, S., Janhunen, P., Koustov, A., Pellinen, R., Danskin, D., & Uspensky, M. (-0001). Stare Velocities: the Importance of Off-orthogonality and Ion Motions : Volume 21, Issue 3 (30/11/-0001). Retrieved from http://hawaiilibrary.net/


Description
Description: Finnish Meteorological Institute, Geophisycal Research, P.O. Box 503, FIN-00101, Helsinki, Finland. A 3.5-h morning event of joint EISCAT/STARE observations is considered and the differences between the observed STARE velocities and the electron drift components (EISCAT) are studied. We find that the STARE-Finland radar velocity was larger than the EISCAT convec-tion component for a prolonged period of time. In addition, a moderate 5–20° offset between the EISCAT convection azimuth and the corresponding STARE estimate was observed. We show that both the STARE-Finland radar velocity "over-speed" and the offset in the azimuth can be explained by fluid plasma theory, if the ion drift contribution to the irregularity phase velocity is taken into account under the condition of a moderate backscatter off-orthogonality. We call such an explanation the off-orthogonal fluid approach (OOFA). In general terms, we found that the azimuth of the maxi-mum irregularity phase velocity Vph is not collinear with the VE × B electron flow direction, but differs by 5–15°. Such an azimuth offset is the key factor, not only for the explanation of the Finland velocity overspeed, but also for the revisions of the velocity cosine rule, traditionally accepted in the STARE method at large flow angles. We argue that such a rule is only a rough approximation. The application of the OOFA to the STARE l-o-s velocities gives a reasonable agreement with the EISCAT convection data, implying that ion motions and the non-orthogonality of backscatter are important to consider for VHF auroral echoes. The data set discussed had the STARE velocity magnitudes, which were 1.5–2 times smaller than the electron VE × B velocities, as was found earlier by Nielsen and Schlegel (1983).

Key words. Ionospheric irregularities; plasma waves and instabilities; auroral ionosphere


Summary
STARE velocities: the importance of off-orthogonality and ion motions

 

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