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Density irregularities in the plasmasphere boundary layer: Cluster observations in the dusk sector
DOI: 10.1016/j.asr.2005.08.050 Bibcode: 2005AdSpR..36.1964D

André, M.; Décréau, P. M. E.; Canu, P. +7 more

We present observations of plasma density structures crossed by the CLUSTER spacecraft constellation near orbit perigee, with the spacecraft located in the vicinity of the plasmapause boundary. Although the constellation is not arranged as a perfect tetrahedron, the four-point measurements reveal interesting properties of density structures, unkno…

2005 Advances in Space Research
Cluster 18
Multi-point observation of the high-speed flows in the plasma sheet
DOI: 10.1016/j.asr.2005.05.101 Bibcode: 2005AdSpR..36.1444N

Balogh, A.; Zhang, T. L.; Klecker, B. +9 more

The structure of the high-speed flows in the midtail plasma sheet is discussed based on results from multi-point observation of Cluster spacecraft in summer 2001 and 2002. The average rate of change in flow speed along the "dawn-dusk" direction (perpendicular to the main flow and in the plane of the tail current sheet) and along the "north-south" …

2005 Advances in Space Research
Cluster 16
Neutral sheet normal direction determination
DOI: 10.1016/j.asr.2004.08.010 Bibcode: 2005AdSpR..36.1940Z

Balogh, A.; Zhang, T. L.; Glassmeier, K. -H. +5 more

One of the important parameters in magnetotail studies is the thickness of the current sheet. The determination of this thickness is subject to many assumptions of the geometry, such as the current sheet normal direction. The minimum variance analysis (MVA) has been widely used in studies of the current sheet in the tail or at the magnetopause wit…

2005 Advances in Space Research
Cluster 12
Analysis of Cluster spacecraft potential during active control
DOI: 10.1016/j.asr.2005.01.110 Bibcode: 2005AdSpR..36.1922T

Escoubet, C. P.; André, M.; Décréau, P. M. E. +4 more

The floating potential of a spacecraft is determined by an equilibrium between photo-electron emission from the sunlit spacecraft surfaces and the plasma electron current, while other currents play a secondary role. On the Cluster spacecraft, the presence of the experiment ASPOC to control the potential by an ion beam with currents up to several t…

2005 Advances in Space Research
Cluster 6
The response of the near earth magnetotail to substorm activity
DOI: 10.1016/j.asr.2004.03.024 Bibcode: 2005AdSpR..36.1818K

Khurana, K. K.; McPherron, R. L.; Thompson, S. +3 more

The large scale structure of the current sheet in the terrestrial magnetotail is often represented as the superposition of a constant northward-oriented magnetic field component ( Bz) and a component along the Earth-Sun direction ( Bx) that varies with distance from the center of the sheet ( z0 in GSM) as in a Hams…

2005 Advances in Space Research
Cluster 6
Cluster observations of magnetospheric substorm behavior in the near- and mid-tail region
DOI: 10.1016/j.asr.2004.04.021 Bibcode: 2005AdSpR..36.1809B

McPherron, R. L.; Dunlop, M. W.; Baker, D. N.

The Cluster constellation of spacecraft has returned substantial new data on particle and field variations in the near- and mid-magnetotail regions of Earth's magnetosphere. Using the Research with Adaptive Particle Imaging Detectors (RAPID) system onboard the four Cluster vehicles, we have identified substorm-related energetic ( E > 20 keV) el…

2005 Advances in Space Research
Cluster 6
Reverse convection and cusp proton aurora: Cluster, polar and image observation
DOI: 10.1016/j.asr.2004.09.023 Bibcode: 2005AdSpR..36.1779Z

Zong, Q. -G.; Daly, P. W.; Mende, S. B. +4 more

On April 21, 2001 an interplanetary CME started to interact with the magnetosphere when CLUSTER spacecraft were travelling in the cusp region. This interaction produced a strong magnetic storm ( Dst = 103 nT) at Earth. Cusp proton aurora was caused by the leading phase of the CME. Cusp proton aurora generally appear during northward IMF…

2005 Advances in Space Research
Cluster 5
Improvement of plasma measurements onboard Cluster due to spacecraft potential control
DOI: 10.1016/j.asr.2005.01.109 Bibcode: 2005AdSpR..36.1951T

Escoubet, C. P.; Dandouras, I.; André, M. +6 more

The ion emitter experiment ASPOC (Active Spacecraft Potential Control) and the plasma electron experiment PEACE (Plasma Electron And Current Experiment) have been operating together in a large variety of plasma environments. Three cases on February 4, 2001, May 21, 2002, and June 12, 2002 have been analysed. A clear improvement of the electron mea…

2005 Advances in Space Research
Cluster 4
What is Cluster telling us about magnetotail dynamics?
DOI: 10.1016/j.asr.2004.02.021 Bibcode: 2005AdSpR..36.1909B

Nakamura, Rumi; Baumjohann, Wolfgang

In this review, we report on some new aspects of magnetotail dynamics found in the data of the first traversal of the magnetotail by the Cluster quartet in summer and autumn 2001: (1) The electron drift instrument made the first direct measurements of tail lobe convection. The statistical data shows convection toward the center of the plasma sheet…

2005 Advances in Space Research
Cluster 2
Energetic particle acceleration during a major magnetic storm
DOI: 10.1016/j.asr.2004.03.023 Bibcode: 2005AdSpR..36.1835K

Grande, M.; Baker, D.; Blake, J. B. +6 more

We study the global properties of energetic (>30 keV) particles during the main and early recovery phase of a major magnetic storm of March 31, 2001, using data of the NOAA 15 and 16 and the CLUSTER satellites. During the storm main phase the ring current energetic electron and ion fluxes were increased by nearly two orders of magnitude, and th…

2005 Advances in Space Research
Cluster 1