Search Publications

Prediction and understanding of the north-south displacement of the heliospheric current sheet
DOI: 10.1029/2004JA010723 Bibcode: 2005JGRA..11010101Z

Hoeksema, J. T.; Scherrer, P. H.; Zhao, X. P.

On the basis of Wilcox Solar Observatory observations of the photospheric magnetic field and the potential field-source surface model, we compare the solid angles occupied by the positive source surface field with that of the negative. We develop an algorithm to quantitatively estimate and understand the positive-negative displacement of the helio…

2005 Journal of Geophysical Research (Space Physics)
Ulysses 35
Orientation and motion of two-dimensional structures in a space plasma
DOI: 10.1029/2004JA010853 Bibcode: 2005JGRA..110.6208S

Hasegawa, H.; Sonnerup, B. U. Ã. -.

We present a new least squares technique for the determination of axis orientation, motion, and intrinsic axial electric field for two-dimensional coherent structures in a space plasma. This single-spacecraft method is based on Faraday's law, which, under the model assumptions, requires the intrinsic axial electric field to be constant in space an…

2005 Journal of Geophysical Research (Space Physics)
Cluster 35
Computing the reconnection rate at the Earth's magnetopause using two spacecraft observations
DOI: 10.1029/2004JA010805 Bibcode: 2005JGRA..110.6212F

RèMe, H.; Owen, C. J.; Fuselier, S. A. +2 more

A new multispacecraft technique is introduced which, under some restrictive assumptions and conditions, provides a snapshot of the reconnection inflow velocity into the magnetosphere and an estimate of the distance from the spacecraft to the reconnection site. The two quantities are not obtained independent of one another and additional, independe…

2005 Journal of Geophysical Research (Space Physics)
Cluster 35
Examination of type II origin with SOHO/LASCO observations
DOI: 10.1029/2004JA010744 Bibcode: 2005JGRA..11012101C

Cho, K. -S.; Kim, Y. -H.; Moon, Y. -J. +5 more

We examine a possibility that metric type II solar radio bursts are all caused by coronal mass ejection (CME) generated shocks. For this we consider 129 type II flare events from February 1997 to October 2000 and examine their associations with SOHO/LASCO CMEs according to their temporal and spatial closeness using SOHO/EIT and GOES data. We then …

2005 Journal of Geophysical Research (Space Physics)
SOHO 34
Nonlinear decay of foreshock Langmuir waves in the presence of plasma inhomogeneities: Theory and Cluster observations
DOI: 10.1029/2004JA010977 Bibcode: 2005JGRA..110.8102S

Krasnoselskikh, V.; Dudok de Wit, T.; Soucek, J. +2 more

The intense high-frequency electrostatic waves observed in the terrestrial foreshock often have a form of a superposition of two monochromatic waves close to the plasma frequency. We suggest an interpretation of these spectra as signatures of nonlinear decay of Langmuir waves to electron-sound and ion-sound secondary waves. This decay instability …

2005 Journal of Geophysical Research (Space Physics)
Cluster 34
October/November 2003 interplanetary coronal mass ejections: ACE/EPAM solar energetic particle observations
DOI: 10.1029/2004JA010926 Bibcode: 2005JGRA..110.9S06M

Lario, D.; Lanzerotti, L. J.; Sarris, E. T. +3 more

In late October and early November 2003 the ACE spacecraft at 1 AU detected two shock-associated interplanetary coronal mass ejections (ICMEs). In the sheath region formed in front of both ICMEs, some of the highest speeds ever directly measured in the solar wind were observed. We analyze in detail the energetic particle signatures measured at 1 A…

2005 Journal of Geophysical Research (Space Physics)
SOHO 34
Solar wind from the coronal hole boundaries
DOI: 10.1029/2004JA010896 Bibcode: 2005JGRA..110.4104S

Geiss, J.; McComas, D. J.; Schwadron, N. A. +3 more

Recent studies using in situ observations established that the interface between fast and slow wind in interplanetary space has two distinct parts: a smoothly varying boundary layer flow that flanks fast wind from coronal holes and a sharper plasma discontinuity between intermediate and slow solar wind. Other studies using in situ observations and…

2005 Journal of Geophysical Research (Space Physics)
Ulysses 34
Dynamic Harris current sheet thickness from Cluster current density and plasma measurements
DOI: 10.1029/2004JA010714 Bibcode: 2005JGRA..110.2212T

Balogh, A.; Khurana, K. K.; Kistler, L. M. +5 more

We use the first accurate measurements of current densities in the plasma sheet to calculate the half-thickness and position of the current sheet as a function of time. Our technique assumes a Harris current sheet model, which is parameterized by lobe magnetic field B0, current sheet half-thickness h, and current sheet position z0<…

2005 Journal of Geophysical Research (Space Physics)
Cluster 33
Interplanetary conditions and magnetospheric dynamics during the Cassini orbit insertion fly-through of Saturn's magnetosphere
DOI: 10.1029/2005JA011054 Bibcode: 2005JGRA..11010212J

Jackman, C. M.; Kurth, W. S.; Cecconi, B. +5 more

The primary purpose of this paper is to discuss the interplanetary conditions that prevailed during the Saturn orbit insertion (SOI) fly-through of Saturn's magnetosphere by the Cassini spacecraft in June-July 2004 and the consequent magnetospheric dynamics. We begin by examining concurrent interplanetary magnetic field (IMF) and Saturn kilometric…

2005 Journal of Geophysical Research (Space Physics)
Cassini 31
On the generation of enhanced sunward convection and transpolar aurora in the high-latitude ionosphere by magnetic merging
DOI: 10.1029/2005JA011149 Bibcode: 2005JGRA..11011218E

Balogh, A.; RèMe, H.; Dunlop, M. W. +11 more

The IMAGE Wideband Imaging Camera (WIC) instrument observed the duskside development of an oval-aligned transpolar auroral arc (TPA) in the Northern Hemisphere (NH) on 16 December 2001 during strong IMF ∣B∣ ∼ 18 nT and a generally steady ∼56° clock angle (positive IMF By and Bz). Observational evidence suggests that the daysi…

2005 Journal of Geophysical Research (Space Physics)
Cluster 31