A flux transfer event observed at the magnetopause by the Equator-S spacecraft and in the ionosphere by the CUTLASS HF radar |
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Authors: | D. A. Neudegg T. K. Yeoman S. W. H. Cowley G. Provan G. Haerendel W. Baumjohann U. Auster K.-H. Fornacon E. Georgescu C. J. Owen |
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Affiliation: | (1) Department of Physics and Astronomy, Leicester University, University Road, Leicester, LE1 7RH, UK;(2) Max-Planck Institut für Extraterrestrische Physik, Garching, Munich, Germany;(3) Technische Universität von Braunschweig, Braunschweig, Germany;(4) ISS, Bucharest, Romania;(5) Queen Mary and Westfield College, Lndon, UK |
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Abstract: | Observations of a flux transfer event (FTE) have been made simultaneously by the Equator-S spacecraft near the dayside magnetopause whilst corresponding transient plasma flows were seen in the near-conjugate polar ionosphere by the CUTLASS Finland HF radar. Prior to the occurrence of the FTE, the magnetometer on the WIND spacecraft ≈226 RE upstream of the Earth in the solar wind detected a southward turning of the interplanetary magnetic field (IMF) which is estimated to have reached the subsolar magnetopause ≈77 min later. Shortly afterwards the Equator-S magnetometer observed a typical bipolar FTE signature in the magnetic field component normal to the magnetopause, just inside the magnetosphere. Almost simultaneously the CUTLASS Finland radar observed a strong transient flow in the F region plasma between 78° and 83° magnetic latitude, near the ionospheric region predicted to map along geomagnetic field lines to the spacecraft. The flow signature (and the data set as a whole) is found to be fully consistent with the view that the FTE was formed by a burst of magnetopause reconnection. |
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Keywords: | Interplanetary physics (ionosphere-magnetosphere interaction) Magnetospheric physics (magnetopause, cusp, and boundary layers solar wind-magnetosphere interactions) |
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