Search Publications

Correlation properties of magnetosheath magnetic field fluctuations
DOI: 10.1029/2009JA014173 Bibcode: 2009JGRA..114.8207G

Němeček, Z.; Gutynska, O.; Šafránková, J.

The magnetosheath is characterized by a variety of low-frequency fluctuations, but their features and sources are different. Taking advantage of multipoint magnetic field measurements of the Cluster spacecraft, we present a statistical study to reveal properties of waves. We compute cross-correlation coefficients of magnetic field strengths as mea…

2009 Journal of Geophysical Research (Space Physics)
Cluster 19
Source region of the 18 November 2003 coronal mass ejection that led to the strongest magnetic storm of cycle 23
DOI: 10.1029/2008JA013845 Bibcode: 2009JGRA..114.3107S

Srivastava, Nandita; Mathew, Shibu K.; Louis, Rohan E. +1 more

The superstorm of 20 November 2003 was associated with a high-speed coronal mass ejection (CME) which originated in the NOAA AR 10501 on 18 November. This coronal mass ejection had severe terrestrial consequences leading to a geomagnetic storm with Dst index of -472 nT, the strongest of the current solar cycle. In this paper, we attempt to underst…

2009 Journal of Geophysical Research (Space Physics)
SOHO 19
Reformation of an oblique shock observed by Cluster
DOI: 10.1029/2009JA014268 Bibcode: 2009JGRA..11411107L

Lucek, E. A.; Schwartz, S. J.; Mazelle, C. +2 more

On 16 March 2005, the Cluster spacecraft crossed a shock almost at the transition between the quasi-perpendicular and quasi-parallel regimes ($\theta$Bn = 46°) preceded by an upstream low-frequency (≈0.02 Hz in the spacecraft frame) wave train observed for more than 10 mn. The wave semicycle nearest to the shock was found to grow in tim…

2009 Journal of Geophysical Research (Space Physics)
Cluster 18
Reconstruction of two-dimensional coherent structures in ideal and resistive Hall MHD: The theory
DOI: 10.1029/2008JA013897 Bibcode: 2009JGRA..114.4206S

Sonnerup, Bengt U. Ö.; Teh, Wai-Leong

We demonstrate that it is possible, in principle, to use data from a single spacecraft to produce reconstructions of two-dimensional, time-independent field and plasma structures in space, in circumstances where the Hall effect is important. Such reconstruction generates maps, in a limited region around the spacecraft path, of magnetic and electri…

2009 Journal of Geophysical Research (Space Physics)
Cluster 18
Determining ion production rates near Saturn's extended neutral cloud from ion cyclotron wave amplitudes
DOI: 10.1029/2008JA013664 Bibcode: 2009JGRA..114.4219C

Russell, C. T.; Tokar, R. L.; Omidi, N. +2 more

Recent Cassini observations of active venting of water molecules from Enceladus indicate that the moon is the primary source of Saturn's extended neutral cloud. Ionization of the neutrals through charge exchange creates a population of newborn ions with a velocity space distribution, which is highly unstable to the generation of electromagnetic io…

2009 Journal of Geophysical Research (Space Physics)
Cassini 17
Quantitative forecasting of near-term solar activity and upper atmospheric density
DOI: 10.1029/2009JA014285 Bibcode: 2009JGRA..114.7301L

Lean, J. L.; Picone, J. M.; Emmert, J. T.

Autoregressive algorithms are developed to forecast solar activity on timescales of 1 to 10 days and utilized to forecast upper atmospheric densities using the NRLMSIS density specification model. Quantitative assessment of solar activity observations and forecasts made over 27 years (from 1980 to 2006) indicates that the chromospheric Mg index is…

2009 Journal of Geophysical Research (Space Physics)
SOHO 17
Hybrid simulations of magnetic reconnection initiated in the magnetosheath
DOI: 10.1029/2008JA013647 Bibcode: 2009JGRA..114.2222O

Omidi, N.; Sibeck, D. G.; Phan, T.

Interaction of solar wind tangential discontinuities (TDs) with the bow shock may initiate reconnection in the magnetosheath. We employ 2.5-D electromagnetic, hybrid simulations that treat the ions kinetically via particle-in-cell methods and the electrons as a massless fluid to study this interaction. We present results from eight runs correspond…

2009 Journal of Geophysical Research (Space Physics)
Cluster 16
Hybrid simulation of foreshock waves and ion spectra and their linkage to cusp energetic ions
DOI: 10.1029/2008JA013745 Bibcode: 2009JGRA..114.6203W

Wang, X. Y.; Lin, Y.; Chang, S. -W.

A three-dimensional global hybrid simulation is carried out to investigate energetic ions and electromagnetic waves in the quasi-parallel (Q-$\parallel$) bow shock and cusp for a typical interplanetary magnetic field configuration during the cusp energetic particle events. The bow shock, magnetosheath, and dayside magnetosphere form by interaction…

2009 Journal of Geophysical Research (Space Physics)
Cluster 16
A simulation study of particle energization observed by THEMIS spacecraft during a substorm
DOI: 10.1029/2009JA014126 Bibcode: 2009JGRA..114.9204A

Bosqued, Jean-Michel; El-Alaoui, Mostafa; Zhou, Meng +6 more

Energetic ions with hundreds of keV energy are frequently observed in the near-Earth tail during magnetospheric substorms. We examined the sources and acceleration of ions during a magnetospheric substorm on 1 March 2008 by using Time History of Events and Macroscale Interactions during Substorms (THEMIS) and Cluster observations and numerical sim…

2009 Journal of Geophysical Research (Space Physics)
Cluster 16
Convective bursty flows in the near-Earth magnetotail inside 13 RE
DOI: 10.1029/2008JA013125 Bibcode: 2009JGRA..114.2202Z

Dunlop, M. W.; Baumjohann, W.; Carr, C. +8 more

With the 4-s resolution data of the magnetometer and the ion plasma analyzer on Double Star TC-1 from June to November of each year during the period of 2004-2006, we statistically analyzed the occurrence rate of both convective and field-aligned bursty flows (FABFs). In the region -13 RE < X < -9 RE, |Y| < 10 R

2009 Journal of Geophysical Research (Space Physics)
DoubleStar 15