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Double Star TC-1 observations of component reconnection at the dayside magnetopause: a preliminary study

Authors :
Andrew Fazakerley
Chijie Xiao
Iannis Dandouras
Chris Carr
Tiantian Zhang
Xinggong Zhang
T. D. Phan
Z. Y. Huang
Z. X. Liu
H. Rème
Hui Zhang
Malcolm Dunlop
Xuejun Wang
Qiugang Zong
Suiyan Fu
Zuyin Pu
School of Earth and Space Sciences [Beijing]
Peking University [Beijing]
Center for Space Science and Applied Research [Beijing] (CSSAR)
Chinese Academy of Sciences [Beijing] (CAS)
National Astronomical Observatories
Space Science and Technology Department [Didcot] (RAL Space)
STFC Rutherford Appleton Laboratory (RAL)
Science and Technology Facilities Council (STFC)-Science and Technology Facilities Council (STFC)
Center for Space Physics [Boston] (CSP)
Boston University [Boston] (BU)
SAPG
The Blackett Laboratory
Centre d'étude spatiale des rayonnements (CESR)
Observatoire Midi-Pyrénées (OMP)
Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3)
Université Fédérale Toulouse Midi-Pyrénées
Mullard Space Science Laboratory (MSSL)
University College of London [London] (UCL)
Space Sciences Laboratory [Berkeley] (SSL)
University of California [Berkeley]
University of California-University of California
Space Research Institute of Austrian Academy of Sciences (IWF)
Austrian Academy of Sciences (OeAW)
Center for Plasma Physics
Blackett Laboratory
Imperial College London
Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP)
Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3)
Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS)
University of California [Berkeley] (UC Berkeley)
University of California (UC)-University of California (UC)
Source :
Annales Geophysicae, Vol 23, Pp 2889-2895 (2005), Annales Geophysicae, Annales Geophysicae, European Geosciences Union, 2005, 23 (8), pp.2889-2895, Annales Geophysicae, 2005, 23 (8), pp.2889-2895, Scopus-Elsevier
Publication Year :
2005
Publisher :
Copernicus Publications, 2005.

Abstract

International audience; In spring 2004 Double Star TC-1 measured a number of reconnection signatures at the dayside low-latitude magnetopause (MP) when there was a notable By component in the magnetosheath. In a number of events we can show that reconnection was operating nearby TC-1 in the subsolar MP region. In this paper we describe three representative events: (a) event on 21 March 2004 in which the reconnection site can be remotely monitored, the spacecraft was passing by the X-line; (b) event on 12 March 2004 in which TC-1 observed the magnetospheric part of the quadrupolar field, together with a consistent flow reversal; (c) event on 26 March 2004 which occurred for northward IMF, TC-1 observed a reversal of vy across the equatorial MP. In these events the shear angles across the MP were considerably smaller than 180°; a noticeable guide field was present. These observations are consistent with near equatorial component merging, suggesting that component reconnection preferably occurs at the dayside low-latitude MP. There is evidence that when a pronounced magnetic shear across the MP exists in the By component, reconnection may operate at the dayside low-latitude MP for northward IMF Bz.

Details

Language :
English
ISSN :
14320576 and 09927689
Volume :
23
Database :
OpenAIRE
Journal :
Annales Geophysicae
Accession number :
edsair.doi.dedup.....8ffe5162846126cd1a59e9b3d0dbd9f8