Search Publications

Simulation of VLF chorus emissions in the magnetosphere and comparison with THEMIS spacecraft data
DOI: 10.1002/2016JA023057 Bibcode: 2017JGRA..122..166D

Santolík, O.; Demekhov, A. G.; Taubenschuss, U.

We present results of numerical simulations of VLF chorus emissions based on the backward wave oscillator model and compare them with Time History of Events and Macroscale Interactions during Substorms (THEMIS) spacecraft data from the equatorial chorus source region on the early morning side at a radial distance of 6 Earth radii. Specific attenti…

2017 Journal of Geophysical Research (Space Physics)
Cluster 42
Solar wind- and EUV-dependent models for the shapes of the Martian plasma boundaries based on Mars Express measurements
DOI: 10.1002/2017JA024098 Bibcode: 2017JGRA..122.7279R

Barabash, Stas; Holmström, Mats; Futaana, Yoshifumi +1 more

The long operational life (2003-present) of Mars Express (MEX) has allowed the spacecraft to make plasma measurements in the Martian environment over a wide range of upstream conditions. We have analyzed ∼7000 MEX orbits, covering three orders of magnitude in solar wind dynamic pressure, with data from the on board Analyzer of Space Plasmas and En…

2017 Journal of Geophysical Research (Space Physics)
MEx 42
On the Dawn-Dusk Asymmetry of the Kelvin-Helmholtz Instability Between 2007 and 2013
DOI: 10.1002/2017JA024548 Bibcode: 2017JGRA..12211888H

Nykyri, K.; Moore, T. W.; Dimmock, A. P. +2 more

Using data from Time History of Events and Macroscale Interactions during Substorms (THEMIS), a statistical study was performed to determine whether a dawn-dusk asymmetry exists in the occurrence rates of the Kelvin-Helmholtz instability during Parker-Spiral (PS) and Ortho-Parker-Spiral (OPS) orientations of the interplanetary magnetic field (IMF)…

2017 Journal of Geophysical Research (Space Physics)
Cluster 38
Timescales for the penetration of IMF By into the Earth's magnetotail
DOI: 10.1002/2016JA023198 Bibcode: 2017JGRA..122..579B

Milan, S. E.; Fear, R. C.; Grocott, A. +1 more

Previous studies have shown that there is a correlation between the By component of the interplanetary magnetic field (IMF) and the By component observed in the magnetotail lobe and in the plasma sheet. However, studies of the effect of IMF By on several magnetospheric processes have indicated that the By

2017 Journal of Geophysical Research (Space Physics)
Cluster 36
Traveling Foreshocks and Transient Foreshock Phenomena
DOI: 10.1002/2017JA023901 Bibcode: 2017JGRA..122.9148K

Omidi, N.; Blanco-Cano, X.; Kajdič, P. +3 more

We use the multispacecraft capabilities of the Cluster and Time History of Events and Macroscale Interactions during Substorms (THEMIS) missions to show that two types of foreshock may be detected in spacecraft data. One is the global foreshock that appears upstream of the Earth's quasi-parallel bow shock under steady or variable interplanetary ma…

2017 Journal of Geophysical Research (Space Physics)
Cluster 34
The MMS Dayside Magnetic Reconnection Locations During Phase 1 and Their Relation to the Predictions of the Maximum Magnetic Shear Model
DOI: 10.1002/2017JA024488 Bibcode: 2017JGRA..12211991T

Russell, C. T.; Fuselier, S. A.; Strangeway, R. J. +12 more

Several studies have validated the accuracy of the maximum magnetic shear model to predict the location of the reconnection site at the dayside magnetopause. These studies found agreement between model and observations for 74% to 88% of events examined. It should be noted that, of the anomalous events that failed the prediction of the model, 72% s…

2017 Journal of Geophysical Research (Space Physics)
DoubleStar 34
Radial and local time structure of the Saturnian ring current, revealed by Cassini
DOI: 10.1002/2016JA023742 Bibcode: 2017JGRA..122.1803S

Krupp, N.; Dougherty, M. K.; Thomsen, M. F. +6 more

We analyze particle and magnetic field data obtained between July 2004 and December 2013 in the equatorial magnetosphere of Saturn, by the Cassini spacecraft. The radial and local time distribution of the total (thermal and suprathermal) particle pressure and total plasma beta (ratio of particle to magnetic pressure) over radial distances from 5 t…

2017 Journal of Geophysical Research (Space Physics)
Cassini 32
Comparative study of the Martian suprathermal electron depletions based on Mars Global Surveyor, Mars Express, and Mars Atmosphere and Volatile EvolutioN mission observations
DOI: 10.1002/2016JA023205 Bibcode: 2017JGRA..122..857S

André, N.; Fedorov, A.; Sauvaud, J. -A. +16 more

Nightside suprathermal electron depletions have been observed at Mars by three spacecraft to date: Mars Global Surveyor, Mars Express, and the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission. This spatial and temporal diversity of measurements allows us to propose here a comprehensive view of the Martian electron depletions through the firs…

2017 Journal of Geophysical Research (Space Physics)
MEx 31
Occurrence rate of whistler waves in the magnetotail reconnection region
DOI: 10.1002/2016JA023670 Bibcode: 2017JGRA..122.7188H

Sahraoui, F.; Deng, X. H.; Huang, S. Y. +9 more

It has long been suggested that whistler waves play an active role during magnetic reconnection. However, all previous observations were based on case studies and could not give a detailed picture as to where the whistler waves occur in the reconnection region. In this paper, a statistical study by using the Cluster data is performed to investigat…

2017 Journal of Geophysical Research (Space Physics)
Cluster 31
Reformation of rippled quasi-parallel shocks: 2-D hybrid simulations
DOI: 10.1002/2017JA024234 Bibcode: 2017JGRA..122.6385H

Wang, Shui; Huang, Can; Hao, Yufei +3 more

One-dimensional (1-D) hybrid simulations have demonstrated that a quasi-parallel shock is nonstationary and undergoes a reformation process. Recently, two-dimensional (2-D) hybrid simulations have revealed that ripples along the shock front is an inherent property of a quasi-parallel shock. In this paper, we investigate reformation process of a ri…

2017 Journal of Geophysical Research (Space Physics)
Cluster 31