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Annales Geophysicae An interactive open-access journal of the European Geosciences Union
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Volume 20, issue 6
Ann. Geophys., 20, 771-779, 2002
https://doi.org/10.5194/angeo-20-771-2002
© Author(s) 2002. This work is distributed under
the Creative Commons Attribution 3.0 License.
Ann. Geophys., 20, 771-779, 2002
https://doi.org/10.5194/angeo-20-771-2002
© Author(s) 2002. This work is distributed under
the Creative Commons Attribution 3.0 License.

  30 Jun 2002

30 Jun 2002

Strong sunward propagating flow bursts in the night sector during quiet solar wind conditions: SuperDARN and satellite observations

C. Senior1, J.-C. Cerisier1, F. Rich2, M. Lester3, and G. K. Parks4 C. Senior et al.
  • 1Centre d’Etude des Environnements Terrestre et Planétaires (CETP), 4 Avenue de Neptune, 94107 Saint-Maur Cedex, France
  • 2AFRL, Hanscom Air Force Base, MA 01731, USA
  • 3Radio and Space Plasma Physics, Department of Physics and Astronomy, University of Leicester, Leicester LE1 7RH, UK
  • 4Space Sciences Laboratory, University of California Berkeley, Berkeley, CA 94720–7450, USA
  • Correspondence to: J.-C. Cerisier
  • (jean-claude.cerisier@cetp.ipsl.fr)

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.

Key words. Ionosphere (Auroral ionosphere; Ionospheremagnetosphere interactions; Particle precipitation)

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