Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/36670
Title: Strong sunward propagating flow bursts in the night sector during quiet solar wind conditions : SuperDARN and satellite observations
Authors: Senior, C.
Cerisier, J. C.
Rich, F.
Lester, Mark
Parks, G. K.
First Published: 1-Jun-2002
Publisher: Copernicus Publications on behalf of the European Geosciences Union
Citation: Annales Geophysicae, 2002, 20 (6), pp. 771-779 (9)
Abstract: High-time resolution data from the two Iceland SuperDARN HF radars show very strong nightside convection activity during a prolonged period of low geomagnetic activity and northward interplanetary magnetic field (IMF). Flows bursts with velocities ranging from 0.8 to 1.7 km/s are observed to propagate in the sunward direction with phase velocities up to 1.5 km/s. These bursts occur over several hours of MLT in the 20:00–01:00 MLT sector, in the evening-side sunward convection. Data from a simultaneous DMSP pass and POLAR UVI images show a very contracted polar cap and extended regions of auroral particle precipitation from the magnetospheric boundaries. A DMSP pass over the Iceland-West field-of-view while one of these sporadic bursts of enhanced flow is observed, indicates that the flow bursts appear within the plasma sheet and at its outward edge, which excludes Kelvin-Helmholtz instabilities at the magnetopause boundary as the generation mechanism. In the nightside region, the precipitation is more spot-like and the convection organizes itself as clockwise U-shaped structures. We interpret these flow bursts as the convective transport following plasma injection events from the tail into the night-side ionosphere. We show that during this period, where the IMF clock angle is around 70°, the dayside magnetosphere is not completely closed.
DOI Link: 10.5194/angeo-20-771-2002
ISSN: 0992-7689
eISSN: 1432-0576
Links: http://www.ann-geophys.net/20/771/2002/
http://hdl.handle.net/2381/36670
Version: Publisher Version
Status: Peer-reviewed
Type: Journal Article
Rights: Copyright © Author(s) 2002. This work is distributed under the Creative Commons Attribution 3.0 License ( http://creativecommons.org/licenses/by/3.0/ ), which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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