Search Publications

Relationship between solar wind low-energy energetic ion enhancements and large geomagnetic storms
DOI: 10.1029/2003JA010044 Bibcode: 2004JGRA..109.1110S

Smith, Z.; Murtagh, W.; Smithtro, C.

It is well established that energetic ion enhancements (an energetic ion enhancement will hereafter be referred to as an EIE) are partly due to acceleration by interplanetary shocks as the shocks propagate towards Earth and that arrivals of these shocks at Earth are well associated with geomagnetic storms. The observation of EIEs at satellites loc…

2004 Journal of Geophysical Research (Space Physics)
SOHO 30
Flow shear near the boundary of the plasma sheet observed by Cluster and Geotail
DOI: 10.1029/2003JA010174 Bibcode: 2004JGRA..109.5204N

Balogh, A.; RèMe, H.; Fazakerley, A. N. +13 more

We report on the transient strong flow shear (large northward/southward electric field) events accompanied by energetic ion beams and localized field-aligned currents observed at the boundary of the premidnight plasma sheet by Cluster in the Northern Hemisphere and Geotail in the Southern Hemisphere. The events took place associated with plasma sh…

2004 Journal of Geophysical Research (Space Physics)
Cluster 30
Cluster measurements of rapidly moving sources of ELF/VLF chorus
DOI: 10.1029/2003JA010289 Bibcode: 2004JGRA..109.5214I

Gurnett, D. A.; Pickett, J. S.; Inan, U. S. +2 more

The first simultaneous measurements of discrete chorus emissions on multiple spacecraft, realized in the context of the Cluster mission, revealed a rather unexpected frequency difference of around 1 kHz between nearly identical discrete elements observed on different spacecraft [, 2001]. This frequency difference is interpreted herein as a natural…

2004 Journal of Geophysical Research (Space Physics)
Cluster 29
Potential barrier in the electrostatic sheath around a magnetospheric spacecraft
DOI: 10.1029/2004JA010398 Bibcode: 2004JGRA..10912207T

Laakso, H.; Escoubet, P.; Hilgers, A. +4 more

Plasma and field measurements on board magnetospheric spacecraft can be influenced by the spacecraft potential and emitted particles such as photoelectrons and secondary electrons. There exist contradictory requirements for, on one hand, minimizing the spacecraft potential and, on the other hand, minimizing perturbations in the sheath and contamin…

2004 Journal of Geophysical Research (Space Physics)
Cluster 27
New properties of energy-dispersed ions in the plasma sheet boundary layer observed by Cluster
DOI: 10.1029/2003JA010277 Bibcode: 2004JGRA..109.5215K

Lundin, R.; Sauvaud, J. -A.; Escoubet, C. P. +18 more

Using multipoint measurements from the Cluster ion spectrometry instruments and the research with adaptive particle imaging detectors, we identified new properties of multiple energy-dispersed ion structures in the plasma sheet boundary layer (PSBL). On 14 February 2001 at about 4.5 RE midnight local time, the PSBL was highly structured…

2004 Journal of Geophysical Research (Space Physics)
Cluster 26
Energetic magnetospheric oxygen in the magnetosheath and its response to IMF orientation: Cluster observations
DOI: 10.1029/2003JA010312 Bibcode: 2004JGRA..109.7203M

Lundin, R.; Sauvaud, J. -A.; Balogh, A. +17 more

We present Cluster observations made during an outbound orbit on 10 December 2000. After exiting the magnetosphere at midlatitude, Cluster spent a long time skimming the magnetopause moving to lower latitude along an orbit approximately in the ZYGSM plane on the dusk flank of the magnetopause. During this time, magnetospheric oxygen wit…

2004 Journal of Geophysical Research (Space Physics)
Cluster 25
Orientation and motion of a discontinuity from single-spacecraft measurements of plasma velocity and density: Minimum mass flux residue
DOI: 10.1029/2003JA010230 Bibcode: 2004JGRA..109.3221S

Balogh, A.; Lavraud, B.; Dunlop, M. W. +4 more

A simple analytical solution is presented to the problem of determining the orientation and motion of a one-dimensional discontinuity in plasma velocity and density, measured by a single spacecraft as the discontinuity moves past it. The method developed is called Minimum Massflux Residue (MMR). Illustrations of the method, based on Cluster measur…

2004 Journal of Geophysical Research (Space Physics)
Cluster 24
Energetic neutral atoms from Jupiter measured with the Cassini magnetospheric imaging instrument: Time dependence and composition
DOI: 10.1029/2003JA010120 Bibcode: 2004JGRA..109.9S11M

Krimigis, S. M.; Mitchell, D. G.; Roelof, E. C. +2 more

During the Cassini spacecraft flyby of Jupiter in late 2000/early 2001, the Ion and Neutral Camera (INCA, one of three sensors that make up the Cassini Magnetospheric Imaging Instrument (MIMI)) obtained the first ever images of Jupiter's magnetosphere in energetic neutral atom (ENA) flux. These emissions are dominated by hydrogen atoms in the ener…

2004 Journal of Geophysical Research (Space Physics)
Cassini 24
On the evolution of the solar wind between 1 and 5 AU at the time of the Cassini Jupiter flyby: Multispacecraft observations of interplanetary coronal mass ejections including the formation of a merged interaction region
DOI: 10.1029/2003JA010112 Bibcode: 2004JGRA..109.9S03H

Dougherty, M. K.; Young, D. T.; Owens, M. J. +5 more

The Cassini flyby of Jupiter occurred at a time near solar maximum. Consequently, the pre-Jupiter data set reveals clear and numerous transient perturbations to the Parker Spiral solar wind structure. Limited plasma data are available at Cassini for this period due to pointing restrictions imposed on the instrument. This renders the identification…

2004 Journal of Geophysical Research (Space Physics)
Cassini SOHO 23
Derivation of electric potential patterns in the inner magnetosphere from Cluster EDI data: Initial results
DOI: 10.1029/2003JA010319 Bibcode: 2004JGRA..10910202M

Torbert, R. B.; Matsui, H.; Quinn, J. M. +2 more

Electric potential patterns are derived in the inner magnetosphere at 4 < L < 10 using 2 years of data from the Electron Drift Instrument (EDI) on Cluster. First, we examine the relations between the electric field and the following three parameters to understand how the potential patterns are organized: BZ component of the interp…

2004 Journal of Geophysical Research (Space Physics)
Cluster 23