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Planetary Period Oscillations in Saturn's Magnetosphere: Cassini Magnetic Field Observations Over the Northern Summer Solstice Interval
DOI: 10.1029/2018JA025237 Bibcode: 2018JGRA..123.3859P

Dougherty, M. K.; Cowley, S. W. H.; Bunce, E. J. +3 more

We determine properties of Saturn's planetary period oscillations from Cassini magnetic measurements over the 2-year interval from September 2015 to end of mission in September 2017, spanning Saturn northern summer solstice in May 2017. Phases of the northern system oscillations are derived over the whole interval, while those of the southern syst…

2018 Journal of Geophysical Research (Space Physics)
Cassini 35
Electromagnetic Electron Cyclotron Instability in the Solar Wind
DOI: 10.1002/2017JA024759 Bibcode: 2018JGRA..123....6L

Lazar, M.; Yoon, P. H.; López, R. A. +1 more

The abundant reports on the existence of electromagnetic high-frequency fluctuations in space plasmas have increased the expectations that theoretical modeling may help understand their origins and implications (e.g., kinetic instabilities and dissipation). This paper presents an extended quasi-linear approach of the electromagnetic electron cyclo…

2018 Journal of Geophysical Research (Space Physics)
Cluster 34
Long-Lasting Poloidal ULF Waves Observed by Multiple Satellites and High-Latitude SuperDARN Radars
DOI: 10.1029/2018JA026003 Bibcode: 2018JGRA..123.8422S

Shi, X.; Nishimura, Y.; Angelopoulos, V. +6 more

Poloidal ultralow frequency (ULF) waves between 5 and 10 mHz were observed by multiple satellites and three high-latitude Super Dual Auroral Radar Network radars during the recovery phase of a moderate geomagnetic storm on 24-27 January 2016. The long-lasting ULF waves were observed in the magnetic field and energetic particle flux perturbations d…

2018 Journal of Geophysical Research (Space Physics)
Cluster 34
Large-Scale Survey of the Structure of the Dayside Magnetopause by MMS
DOI: 10.1002/2017JA025121 Bibcode: 2018JGRA..123.2018P

Russell, C. T.; Lavraud, B.; Baumjohann, W. +13 more

This paper describes the generation and initial utilization of a database containing 80 vector and scalar quantities, for a total of 8,670 magnetopause and magnetosheath current sheet crossings by MMS1, using plasma and magnetic field data from the Fast Plasma Investigation, Fluxgate Magnetometer, and Hot Plasma Composition Analyzer instruments, a…

2018 Journal of Geophysical Research (Space Physics)
Cluster 31
How the IMF By Induces a Local By Component During Northward IMF Bz and Characteristic Timescales
DOI: 10.1002/2018JA025186 Bibcode: 2018JGRA..123.3333T

Snekvik, K.; Østgaard, N.; Tenfjord, P. +7 more

We use the Lyon-Fedder-Mobarry global magnetohydrodynamics model to study the effects of the interplanetary magnetic field (IMF) By component on the coupling between the solar wind and magnetosphere-ionosphere system when IMF Bz>0. We describe the evolution of how a magnetospheric By component is induced on clos…

2018 Journal of Geophysical Research (Space Physics)
Cluster 26
Oxygen Ion Energization at Mars: Comparison of MAVEN and Mars Express Observations to Global Hybrid Simulation
DOI: 10.1002/2017JA024884 Bibcode: 2018JGRA..123.1678J

Fedorov, A.; Holmström, M.; Modolo, R. +2 more

We study oxygen ion energization in the Mars-solar wind interaction by comparing particle and magnetic field observations on the Mars Atmosphere and Volatile EvolutioN (MAVEN) and Mars Express missions to a global hybrid simulation. We find that large-scale structures of the Martian-induced magnetosphere and plasma environment as well as the Mars …

2018 Journal of Geophysical Research (Space Physics)
MEx 26
Global MHD Simulations of the Earth's Bow Shock Shape and Motion Under Variable Solar Wind Conditions
DOI: 10.1002/2017JA024690 Bibcode: 2018JGRA..123..259M

Eastwood, J. P.; Schwartz, S. J.; Mejnertsen, L. +2 more

Empirical models of the Earth's bow shock are often used to place in situ measurements in context and to understand the global behavior of the foreshock/bow shock system. They are derived statistically from spacecraft bow shock crossings and typically treat the shock surface as a conic section parameterized according to a uniform solar wind ram pr…

2018 Journal of Geophysical Research (Space Physics)
Cluster 25
Evidence for Auroral Emissions From Callisto's Footprint in HST UV Images
DOI: 10.1002/2017JA024791 Bibcode: 2018JGRA..123..364B

Gérard, Jean-Claude; Clarke, John T.; Grodent, Denis +3 more

Auroral emissions are expected from the footprint of Callisto in Jupiter's upper atmosphere owing to the known interaction of its atmosphere with Jupiter's magnetosphere, and from the observed auroral emissions from the footprints of the other three Galilean satellites. The mapping of Callisto along modeled magnetic field lines at Jupiter, however…

2018 Journal of Geophysical Research (Space Physics)
eHST 24
Ionospheric Irregularities at Mars Probed by MARSIS Topside Sounding
DOI: 10.1002/2017JA024913 Bibcode: 2018JGRA..123.1018H

Gurnett, D. A.; Halekas, J. S.; Kopf, A. J. +2 more

The upper ionosphere of Mars contains a variety of perturbations driven by solar wind forcing from above and upward propagating atmospheric waves from below. Here we explore the global distribution and variability of ionospheric irregularities around the exobase at Mars by analyzing topside sounding data from the Mars Advanced Radar for Subsurface…

2018 Journal of Geophysical Research (Space Physics)
MEx 24
Comparison of Dust Impact and Solitary Wave Signatures Detected by Multiple Electric Field Antennas Onboard the MMS Spacecraft
DOI: 10.1029/2018JA025380 Bibcode: 2018JGRA..123.6119V

Mann, Ingrid; Vaverka, Jakub; Pellinen-Wannberg, Asta +6 more

Dust impact detection by electric field instruments is a relatively new method. However, the influence of dust impacts on electric field measurements is not completely understood and explained. A better understanding is very important for reliable dust impact identification, especially in environments with low dust impact rate. Using data from Ear…

2018 Journal of Geophysical Research (Space Physics)
Cluster 23