Search Publications

Heliospheric energetic particle observations during the October-November 2003 events
DOI: 10.1029/2004JA010940 Bibcode: 2005JGRA..110.9S11L

Livi, S.; Russell, C. T.; Lario, D. +4 more

The intense level of solar activity recorded from 19 October to 12 November 2003 led to unusually high energetic particle intensities observed throughout the heliosphere. The fleet of spacecraft distributed in the inner and outer heliosphere offers us the opportunity to study both the effects of these events in different regions of the heliosphere…

2005 Journal of Geophysical Research (Space Physics)
Ulysses 38
Reconstruction of the reconnection rate from Cluster measurements: First results
DOI: 10.1029/2005JA011181 Bibcode: 2005JGRA..11011217S

Penz, T.; Kubyshkin, I. V.; Nakamura, R. +6 more

A model of transient time-dependent magnetic reconnection is used to describe the behavior of nightside flux transfers (NFTEs) in the Earth's magnetotail. On the basis of the analytical approach to reconnection developed by Heyn and Semenov (1996) and Semenov et al. (2004a) we calculate the magnetic field and plasma bulk velocity time series obser…

2005 Journal of Geophysical Research (Space Physics)
Cluster 38
Solar energetic electrons related to the 28 October 2003 flare
DOI: 10.1029/2004JA010910 Bibcode: 2005JGRA..110.9S04K

Krucker, S.; Mann, G.; Kunow, H. +4 more

We investigate the solar origin of near-relativistic electrons and protons during the X17.2/4B flare as observed by the Comprehensive Suprathermal and Energetic Particle Analyser (COSTEP) and Three-Dimensional Plasma (3DP) analyzer experiments on board the SOHO and Wind spacecraft. These observations are combined with ground- and space-based spect…

2005 Journal of Geophysical Research (Space Physics)
SOHO 37
The k-filtering technique applied to wave electric and magnetic field measurements from the Cluster satellites
DOI: 10.1029/2005JA011125 Bibcode: 2005JGRA..11011224T

Sahraoui, Fouad; André, Mats; Cornilleau-Wehrlin, Nicole +2 more

The k-filtering technique is a method to characterize stationary fluctuations in space plasmas in terms of the wave energy distribution in the frequency and wave vector space. It has the ability to distinguish between wave modes of the same frequency in the spacecraft frame of reference, but with different wave vectors. This method is based on sim…

2005 Journal of Geophysical Research (Space Physics)
Cluster 36
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