| On the association between energy conversion regions and high speed flows in the plasma sheet | | Octav Marghitu (1), Maria Hamrin (2), Patrik Norqvist (2), Berndt Klecker (3) |
| (1) Institute for Space Sciences, Bucharest, Romania
(2) Department of Physics, Umea University, Sweden
(3) Max Planck Institute for Extraterrestrial Physics, Garching, Germany |
| | Magnetosphere-ionosphere coupling in the Harang region | | Octav Marghitu (1), Costel Bunescu (1), Tomas Karlsson (2), Berndt Klecker (3) |
| (1) Institute for Space Sciences, Bucharest, Romania
(2) Space and Plasma Physics, Royal Institute of Technology, Stockholm, Sweden
(3) Max Planck Institute for Extraterrestrial Physics, Garching, Germany
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| Observed variation in ionospheric outflow during the 11 October 2001 moderate storm | | Jichun Zhang^{1}, Lynn M. Kistler^{1}, Christopher G. Mouikis^{1}, Hiroshi Matsui^{1}, Berndt Klecker^{2}, Iannis Dandouras^{3}, and Malcolm W. Dunlop^{4} |
| ^{1}Space Science Center, University of New Hampshire, USA
^{2}Max-Planck-Institut für extraterrestrische Phsik, Germany
^{3}CESR/CNRS, France
^{4}Rutherford Appleton Laboratory, UK |
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| BBF / plasma bubble coupling to the ionosphere | | Colin Forsyth |
| UCL-MSSL |
| | Multi-spacecraft observations of auroral electron acceleration by Cluster | | C. Forsyth (1), A.N. Fazakerley (1), A.P. Walsh (1), K. Garza (1), C.J. Owen (1), I. Dandouras (2,3), K-H. Fornacon (4) |
| (1) UCL MSSL, Dorking UK,
(2) Universite de Toulouse, France,
(3) CNRS, Toulouse, France,
(4) Technische Universität Braunschweig, Germany |
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| Advances in modeling and understanding in-situ observations and coupling of the magnetosphere and the auroral ionosphere during Cluster-DMSP conjunctions | | Marius Echim(1,2), Romain Maggiolo(1), Johan De Keyser(1), Michel Roth(1) |
| (1)Belgian Institute for Space Aeronomy, Brussels, Belgium
(2)Institute for Space Sciences, Magurele, Romania |
| | Kinetic properties of the interface between the solar wind and the
magnetosphere of Venus and Earth: modeling and
observations by Venus Express and Cluster | | Marius M. Echim (1,2), R. Maggiolo (1), J. De Keyser (1), H. Gunell (1), T. Zhang (3),
G. Voitcu (2), R. Lundin (4), and S. Barabash (4) |
| (1) Belgian Institute for Space Aeronomy, Brussels, Belgium (2) Institute for Space Sciences, Bucharest,
Romania, (3) Space Research Institute, Austrian Academy of Sciences, Graz, Austria, (4)Swedish Institute for Space
Physics, Kiruna, Sweden |
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| An Interpretation Of The Wave Propagation Properties Observed On WHISPER Passive Mode As An Estimation Of The Electron Density | | Jean-Louis Rauch, Jean-Gabriel Trotignon, Pierrette Décréau Xavier Vallières, Gabor Facsko, Séna Kougblénou, and Guillaume Lointier |
| Laboratoire de Physique et Chimie de l’Environnement et de l’Espace, Centre National de la Recherche Scientifique, LPC2E/CNRS, ORLEANS, France, jean-louis.rauch @cnrs-orleans.fr |
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| Timing method for determining the parameters of a 2-D, non-planar discontinuity | | A. Blagau (1, 2), B. Klecker (2), G. Paschmann (2), S. Haaland (3, 4), O. Marghitu (1), and M. Scholer (2)
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| (1) Institute for Space Sciences, Bucharest, Romania.
(2) MPE, Garching, Germany.
(3) MPS, Katlenburg-Lindau, Germany
(4) Department of Physics, University of Bergen, Norway.
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| Anisotropy evolution of magnetic field fluctuation through the bow shock | | Y. Narita [1] and K.-H. Glassmeier [1,2] |
| [1] Institut fuer Geophysik und extraterrestrische Physik,
Technische Universitaet Braunschweig, Mendelssohnstr. 3,
D-38116 Braunschweig, Germany
[2] Max-Planck-Institut fuer Sonnensystemforschung,
Max-Planck-Str. 2, D-37191 Katlenburg-Lindau, Germany |
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| Field-aligned currents in the magnetotail observed by Cluster | | J. K. Shi (1), Z. W. Cheng (1), T. L. Zhang (2), M. Dunlop (3), Z. X. Liu (1), A. Fazakerley (4), E. Lucek (5), H. Reme (6), M. Taylor(7), I. Dandouras (6) |
| (1)State Key Laboratory of Space Weather, CSSAR, Chinese Academy of Sciences, Beijing, China
(2)Space Research Institute, Austrian Academy of Sciences, Graz, Austria
(3)SSTD, Rutherford Appleton Laboratory, Chilton, Didcot, UK.
(4)MSSL, University College London, UK
(5)Imperial College London, UK
(6)University of Toulouse, UPS, CESR, and CNRS, Toulouse, France
(7)European Space Technology Centre, Noordwijk, The Netherlands
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| Study of the auroral current-voltage relationship using Cluster electric field and particle data | | Mykhaylo Hayosh (1), Octav Marghitu (2), Tomas Karlsson (3) |
| (1) Institute of Atmospheric Physics, Prague, the Czech Republic
(2) Institute for Space Sciences, Bucharest, Romania
(3) Space and Plasma Physics, School of Electrical Engineering, KTH, Stockholm, Sweden. |
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| Estimating the net plasma loss from ionospheric outflow | | S. Haaland [1,2],
E. Engwall [3],
A. Eriksson [3],
M. F"\orster [4],
B. Lybekk [5],
A. Pedersen [5],
K. Svenes [6] |
| [1] Max-Planck Institute for Solar Systems Research, Germany
[2] University of Bergen, Norway
[3] Swedish Institute of Space Physics , Uppsala, Sweden
[4] Helmholtz-Zentrum Potsdam, GFZ German Research Centre for Geoscienses, Germany
[5] University of Oslo, Norway
[6] Norwegian Defense Research Establishment, Norway
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| Efficient ion heating at high altitude, wave and temperature characteristics | | H. Nilsson (1), M. Waara (1), R. Slapak (1), M. André (2) |
| (1) Swedish Institute of Space Physics, Kiruna
(2) Swedish Institute of Space Physics, Uppsala |
| | Heavy ion energization, transport, and loss at Earth, Mars, and Venus | | H. Nilsson |
| Swedish Institute of Space Physics |
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| Low Frequency Waves in and around Energy Conversion Regions in the Plasma Sheet | | D. Constantinescu (1,2)
O. Marghitu (2)
M. Hamrin (3)
K.-H. Glassmeier
|
| (1) Institute for Geophysics and Extraterrestrial Physics, TU Braunschweig, Braunschweig, Niedersachsen, Germany.
(2) Institute for Space Sciences, Bucharest, Romania.
(3) Faculty of Science and Technology, Umea University, Umea, Sweden.
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| First WBD Results from the Winter 2009/2010 Auroral Acceleration Region Campaign | | I. Christopher (1), R. Mutel (1), J. Pickett (1), A. Fazakerley (2), C. Forsyth (2), A. Masson (3), E. Lucek (4)
|
| (1) University of Iowa, Iowa City, USA
(2) UCL MSSL, Dorking, UK
(3) ESA/ESTEC, Noordwijk, The Netherlands
(4) Imperial College, London, UK |
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| Influence of the Field Aligned Beam on the Scattering of Diffuse Iions at the Earth’s Quasi-Parallel Bow Shock | | A. Kis (2), M. Scholer (1), B. Klecker (1), E. A. Lucek (3), H. Rème (4), V. Wesztergom (2), I. Lemperger (2) |
| (1) Max-Planck-Institut für extraterrestrische Physik, Garching, Germany,
(2) Geodetic and Geophysical Research Institute of HAS, Sopron, Hungary,
(3) The Blackett Laboratory, Imperial College, London, UK,
(4) CESR, Toulouse, France, |
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| Polar cap arcs - FAC and ion outflow – Cluster results | | Romain Maggiolo(1), M. Echim(1,2), D. Fontaine(3), A. Teste(4), J. De Keyser(1), C. Jacquey(5) and I. Dandouras(5) |
| (1) Belgian Institute for Space Aeronomy, Space Plasma, Brussels, Belgium, (2) Institute for Space Sciences, Bucharest, Romania (3) Laboratoire de Physique des Plasmas, Velizy, France (4) Space Sciences Laboratory, Berkeley, United States (5) CESR, Université Paul Sabatier, Toulouse, France
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| Use of CLUSTER data in investigating the correspondence between different regions of inner magnetosphere and ionospheric phenomena | | Mirela Voiculescu (1), Viviane Pierrard (2), Fabien Darrouzet (2), Marius Echim (2, 3), Johan De Keyser (2) |
| (1) Dunarea de Jos University of Galati, Romania
(2) Belgian Institute for Space Aeronomie, Brussels, belgium
(3) Institute for Space Sciences, Bucharest, Romania |
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| Current density calculation deep inside the ring current, using the curlometer technique | | S. Grimald (1), I. Dandouras (1), E. Lucek (2), A. N. Fazakerley (3) |
| (1) CESR, Toulouse, France
(2) Imperial Colleg, London, UK
(3) MSSl / UCL, Dorking, UK |
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| Characteristics of storm-time electric fields in the inner magnetosphere | | H. Matsui (1), P. A. Puhl-Quinn (2), J. W. Bonnell (3), C. J. Farrugia (1), V. K. Jordanova (4), Yu. V. Khotyaintsev (5), P.-A. Lindqvist (6), E. Georgescu (7), and R. B. Torbert (1) |
| (1) University of New Hampshire, USA (2) AER, Inc., USA (3) University of California, Berkeley, USA (4) Los Alamos National Laboratory, USA (5) Swedish Institute of Space Physics, Uppsala, Sweden (6) Royal Institute of Technology, Sweden (7) Max-Planck-Institut für Sonnensystemforschung, Germany |
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