Coordinated Cluster, ground-based instrumentation and low-altitude satellite observations of transient poleward-moving events in the ionosphere and in the tail lobe

Lockwood, M. and Opgenoorth, H. J. and van Eyken, A. P. and Fazakerley, A. N. and Bosqued, J. M. and Denig, W. F. and Wild, J. A. and Cully, C. and Greenwald, R. A. and Lu, G. and Amm, O. and Strömme, A. and Prikryl, P. and Hapgood, M. A. and Wild, M. N. and Stamper, R. and Taylor, M. G. G. T. and McCrea, I. W. and Kauristie, K. and Pulkkinen, T. I. and Pitout, F. and Balogh, A. and Dunlop, M. W. and Rème, H. and Behlke, R. and Hansen, T. L. and Provan, G. and Eglitis, P. and Morley, S. K. and Alcaydé, D. and Blelly, P.-L. and Moen, J. and Donovan, E. F. and Engebretson, M. J. and Lester, M. and Watermann, J. F. and Marcucci, M. F. (2001) Coordinated Cluster, ground-based instrumentation and low-altitude satellite observations of transient poleward-moving events in the ionosphere and in the tail lobe. Annales Geophysicae, 19 (10). pp. 1589-1612. ISSN 0992-7689

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During the interval between 8:00–9:30 on 14 January 2001, the four Cluster spacecraft were moving from the central magnetospheric lobe, through the dusk sector mantle, on their way towards intersecting the magnetopause near 15:00 MLT and 15:00 UT. Throughout this interval, the EISCAT Svalbard Radar (ESR) at Longyearbyen observed a series of poleward-moving transient events of enhanced F-region plasma concentration (“polar cap patches”), with a repetition period of the order of 10 min. Allowing for the estimated solar wind propagation delay of 75 (±5)min, the interplanetary magnetic field (IMF) had a southward component during most of the interval. The magnetic footprint of the Cluster spacecraft, mapped to the ionosphere using the Tsyganenko T96 model (with input conditions prevailing during this event), was to the east of the ESR beams. Around 09:05 UT, the DMSP-F12 satellite flew over the ESR and showed a sawtooth cusp ion dispersion signature that also extended into the electrons on the equatorward edge of the cusp, revealing a pulsed magnetopause reconnection. The consequent enhanced ionospheric flow events were imaged by the SuperDARN HF backscatter radars. The average convection patterns (derived using the AMIE technique on data from the magnetometers, the EISCAT and SuperDARN radars, and the DMSP satellites) show that the associated poleward-moving events also convected over the predicted footprint of the Cluster spacecraft. Cluster observed enhancements in the fluxes of both electrons and ions. These events were found to be essentially identical at all four spacecraft, indicating that they had a much larger spatial scale than the satellite separation of the order of 600 km. Some of the events show a correspondence between the lowest energy magnetosheath electrons detected by the PEACE instrument on Cluster (10–20 eV) and the topside ionospheric enhancements seen by the ESR (at 400–700 km). We suggest that a potential barrier at the magnetopause, which prevents the lowest energy electrons from entering the magnetosphere, is reduced when and where the boundary-normal magnetic field is enhanced and that the observed polar cap patches are produced by the consequent enhanced precipitation of the lowest energy electrons, making them and the low energy electron precipitation fossil remnants of the magnetopause reconnection rate pulses.

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Journal Article
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Annales Geophysicae
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24 Jun 2008 17:23
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15 Mar 2024 00:39