Search Publications

Formation of downstream high-speed jets by a rippled nonstationary quasi-parallel shock: 2-D hybrid simulations
DOI: 10.1002/2015JA021419 Bibcode: 2016JGRA..121.2080H

Lu, Q.; Lembege, B.; Hao, Y. +1 more

Experimental observations from space missions (including more recently Cluster and Time History of Events and Macroscale Interactions during Substorms data) have clearly revealed the existence of high-speed jets (HSJs) in the downstream region of the quasi-parallel terrestrial bow shock. Presently, two-dimensional hybrid simulations are performed …

2016 Journal of Geophysical Research (Space Physics)
Cluster 43
Origin of low proton-to-electron temperature ratio in the Earth's plasma sheet
DOI: 10.1002/2016JA022874 Bibcode: 2016JGRA..121.9985G

Zelenyi, L. M.; Sauvaud, J. -A.; Lavraud, B. +4 more

We study the proton-to-electron temperature ratio (Tp/Te) in the plasma sheet (PS) of the Earth's magnetotail using 5 years of Cluster observations (2001-2005). The PS intervals are searched within a region defined with -19 < X ≤ -7 RE and |Y| < 15 RE (GSM) under the condition |BX| ≤ 10 …

2016 Journal of Geophysical Research (Space Physics)
Cluster 40
On the propagation of a geoeffective coronal mass ejection during 15-17 March 2015
DOI: 10.1002/2016JA022924 Bibcode: 2016JGRA..121.7423W

Webb, D. F.; Wang, Yuming; Shen, Fang +11 more

The largest geomagnetic storm so far, called 2015 St. Patrick's Day event, in the solar cycle 24 was produced by a fast coronal mass ejection (CME) originating on 15 March 2015. It was an initially west-oriented CME and expected to only cause a weak geomagnetic disturbance. Why did this CME finally cause such a large geomagnetic storm? We try to f…

2016 Journal of Geophysical Research (Space Physics)
SOHO VenusExpress 40
Four-fluid MHD simulations of the plasma and neutral gas environment of comet 67P/Churyumov-Gerasimenko near perihelion
DOI: 10.1002/2015JA022333 Bibcode: 2016JGRA..121.4247H

Hansen, Kenneth C.; Gombosi, Tamas I.; Combi, Michael R. +9 more

The neutral and plasma environment is critical in understanding the interaction of the solar wind and comet 67P/Churyumov-Gerasimenko (CG), the target of the European Space Agency's Rosetta mission. To serve this need and support the Rosetta mission, we have developed a 3-D four-fluid model, which is based on BATS-R-US (Block-Adaptive Tree Solarwi…

2016 Journal of Geophysical Research (Space Physics)
Rosetta 40
Properties of current sheet thinning at x ∼- 10 to -12 RE
DOI: 10.1002/2016JA022779 Bibcode: 2016JGRA..121.6718A

Artemyev, A. V.; Runov, A.; Angelopoulos, V. +1 more

We report on Time History of Events and Macroscale Interactions during Substorms (THEMIS) observations of current sheet thinning in Earth's magnetotail at around x =- 10 to -12 Earth radii. The THEMIS spacecraft configuration in October-December 2015 allows us to construct both gradients that contribute to the cross-tail current density jy=µ…

2016 Journal of Geophysical Research (Space Physics)
Cluster 39
A statistical study of plasmaspheric plumes and ionospheric outflows observed at the dayside magnetopause
DOI: 10.1002/2015JA021540 Bibcode: 2016JGRA..121..492L

Zhang, H.; Zong, Q. -G.; Rème, H. +3 more

We present a statistical study of plasmaspheric plumes and ionospheric outflows observed by the Cluster spacecraft near the dayside magnetopause. Plasmaspheric plumes are identified when the low-energy ions (<1 keV) with ∼90° pitch angle distributions are observed by the Cluster Ion Spectrometer/Hot Ion Analyzer instrument. The ionospheric outf…

2016 Journal of Geophysical Research (Space Physics)
Cluster 37
Observation of an MHD Alfvén vortex in the slow solar wind
DOI: 10.1002/2015JA022248 Bibcode: 2016JGRA..121.3870R

Alexandrova, O.; Li, B.; Li, X. +1 more

In the solar wind, magnetic field power spectra usually show several power laws. In this paper, magnetic field data from the Cluster mission during an undisturbed interval of slow solar wind are analyzed at 0.28 Hz, near the spectral break point between the ion inertial and dissipation/dispersion ranges. Assuming Taylor's frozen-in condition, it c…

2016 Journal of Geophysical Research (Space Physics)
Cluster 35
Solar wind interaction with comet 67P: Impacts of corotating interaction regions
DOI: 10.1002/2015JA022147 Bibcode: 2016JGRA..121..949E

Glassmeier, K. -H.; Nilsson, H.; Henri, P. +18 more

We present observations from the Rosetta Plasma Consortium of the effects of stormy solar wind on comet 67P/Churyumov-Gerasimenko. Four corotating interaction regions (CIRs), where the first event has possibly merged with a coronal mass ejection, are traced from Earth via Mars (using Mars Express and Mars Atmosphere and Volatile EvolutioN mission)…

2016 Journal of Geophysical Research (Space Physics)
Rosetta 34
Empirical model of the Martian dayside ionosphere: Effects of crustal magnetic fields and solar ionizing flux at higher altitudes
DOI: 10.1002/2015JA022060 Bibcode: 2016JGRA..121.1760N

Gurnett, D. A.; Němec, F.; Morgan, D. D. +1 more

We use electron density profiles measured by the Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument on board the Mars Express spacecraft to investigate the effects of possible controlling parameters unconsidered in the empirical model of Němec et al. (2011, hereafter N11). Specifically, we focus on the effects of crustal magneti…

2016 Journal of Geophysical Research (Space Physics)
MEx 34
In situ observations of flux rope at the separatrix region of magnetic reconnection
DOI: 10.1002/2015JA021468 Bibcode: 2016JGRA..121..205H

Vaivads, A.; Retino, A.; Sahraoui, F. +12 more

We present the first in situ observations of a small-scale flux rope locally formed at the separatrix region of magnetic reconnection without large guide field. Bidirectional electron beams (cold and hot beams) and density cavity accompanied by intense wave activity substantiate the crossing of the separatrix region. Density compression and one pa…

2016 Journal of Geophysical Research (Space Physics)
Cluster 34