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Variation of Jupiter's aurora observed by Hisaki/EXCEED: 2. Estimations of auroral parameters and magnetospheric dynamics
DOI: 10.1002/2015JA021272 Bibcode: 2016JGRA..121.4055T

Tsuchiya, Fuminori; André, Nicolas; Fujimoto, Masaki +7 more

Jupiter's auroral parameters are estimated from observations by a spectrometer EXCEED (Extreme Ultraviolet Spectroscope for Exospheric Dynamics) on board Japanese Aerospace Exploration Agency's Earth-orbiting planetary space telescope Hisaki. EXCEED provides continuous auroral spectra covering the wavelength range over 80-148 nm from the whole nor…

2016 Journal of Geophysical Research (Space Physics)
eHST 28
Mirror modes in the Earth's magnetosheath: Results from a global hybrid-Vlasov simulation
DOI: 10.1002/2015JA022026 Bibcode: 2016JGRA..121.4191H

Vainio, Rami; Pfau-Kempf, Yann; Ganse, Urs +5 more

We investigate mirror mode structures in the Earth's magnetosheath using our global kinetic Vlasiator simulation, which models ion behavior through their distribution function and treats electrons as a charge-neutralizing fluid. We follow the evolution of waves as they advect along velocity streamlines through the magnetosheath. We find that mirro…

2016 Journal of Geophysical Research (Space Physics)
Cluster 28
Reconstructing the magnetosphere from data using radial basis functions
DOI: 10.1002/2015JA022242 Bibcode: 2016JGRA..121.2249A

Tsyganenko, Nikolai A.; Andreeva, Varvara A.

A new method is proposed to derive from data magnetospheric magnetic field configurations without any a priori assumptions on the geometry of electric currents. The approach utilizes large sets of archived satellite data and uses an advanced technique to represent the field as a sum of toroidal and poloidal parts, whose generating potentials Ψ

2016 Journal of Geophysical Research (Space Physics)
Cluster 28
DC and low-frequency double probe electric field measurements in space
DOI: 10.1002/2016JA022952 Bibcode: 2016JGRA..12110942M

Mozer, F. S.

The double probe technique for measuring DC and low-frequency electric fields in space plasmas is described with an emphasis on uncertainties in the measurements, data analysis techniques, and methods for improving the electric field measurements in future missions.

2016 Journal of Geophysical Research (Space Physics)
Cluster 26
Reconnection events in Saturn's magnetotail: Dependence of plasmoid occurrence on planetary period oscillation phase
DOI: 10.1002/2015JA021985 Bibcode: 2016JGRA..121.2922J

Jackman, C. M.; Cowley, S. W. H.; Provan, G.

During its exploration of Saturn's magnetotail the Cassini magnetometer has detected many in situ examples of magnetic reconnection, in the form of plasmoids, traveling compression regions (TCRs), and dipolarizations. Meanwhile, many magnetospheric phenomena have been shown to be organized with particular regularity by planetary period oscillation…

2016 Journal of Geophysical Research (Space Physics)
Cassini 25
Auroral evidence of radial transport at Jupiter during January 2014
DOI: 10.1002/2016JA023007 Bibcode: 2016JGRA..121.9972G

Gray, R. L.; Badman, S. V.; Bonfond, B. +5 more

We present Jovian auroral observations from the 2014 January Hubble Space Telescope (HST) campaign and investigate the auroral signatures of radial transport in the magnetosphere alongside contemporaneous radio and Hisaki EUV data. HST FUV auroral observations on day 11 show, for the first time, a significantly superrotating polar spot poleward of…

2016 Journal of Geophysical Research (Space Physics)
eHST 25
Global magnetohydrodynamic simulation of the 15 March 2013 coronal mass ejection event—Interpretation of the 30-80 MeV proton flux
DOI: 10.1002/2015JA021051 Bibcode: 2016JGRA..121...56W

Wu, S. T.; Vourlidas, Angelos; Wu, Chin-Chun +4 more

The coronal mass ejection (CME) event on 15 March 2013 is one of the few solar events in Cycle 24 that produced a large solar energetic particle (SEP) event and severe geomagnetic activity. Observations of SEP from the ACE spacecraft show a complex time-intensity SEP profile that is not easily understood with current empirical SEP models. In this …

2016 Journal of Geophysical Research (Space Physics)
SOHO 22
Ionospheric loss from Mars as predicted by hybrid particle simulations
DOI: 10.1002/2016JA022548 Bibcode: 2016JGRA..12110190B

Brecht, Stephen H.; Ledvina, Stephen A.; Bougher, Stephen W.

This paper reports the results of hybrid simulations of the Mars-solar wind interaction. The focus is on the loss rates of O+ and O2+ from the Martian ionosphere while examining the importance of including 3-D dimensional neutral atmospheres with their associated neutral winds. The simulation loss rates are found t…

2016 Journal of Geophysical Research (Space Physics)
MEx 22
A survey of superthermal electron flux depressions, or "electron holes," within the illuminated Martian induced magnetosphere
DOI: 10.1002/2015JA021866 Bibcode: 2016JGRA..121.4835H

Fränz, M.; Lester, M.; Andrews, D. J. +4 more

Since Mars lacks a global intrinsic magnetic field, the solar wind interacts directly with the Martian upper atmosphere and ionosphere. The presence of localized intense remnant crustal magnetic fields adds to this interaction, making the Martian plasma system a unique environment within the solar system. Rapid reductions in the electron flux, ref…

2016 Journal of Geophysical Research (Space Physics)
MEx 22
Oxygen impacts on dipolarization fronts and reconnection rate
DOI: 10.1002/2015JA021747 Bibcode: 2016JGRA..121.1148L

Lapenta, Giovanni; Walker, Raymond J.; Ashour-Abdalla, Maha +1 more

Spacecraft observations near a magnetotail X line show that oxygen (O+) ions are minor species during nonstorm substorms, but they can become major species during some of the storm time substorms. Dipolarization fronts (DFs), which are characterized by a sharp increase northward magnetic field in the magnetotail, are commonly observed d…

2016 Journal of Geophysical Research (Space Physics)
Cluster 22