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Generic Magnetic Field Intensity Profiles of Interplanetary Coronal Mass Ejections at Mercury, Venus, and Earth From Superposed Epoch Analyses
DOI: 10.1029/2018JA025949 Bibcode: 2019JGRA..124..812J

Lugaz, Noé; Möstl, Christian; Janvier, Miho +8 more

We study interplanetary coronal mass ejections (ICMEs) measured by probes at different heliocentric distances (0.3-1 AU) to investigate the propagation of ICMEs in the inner heliosphere and determine how the generic features of ICMEs change with heliospheric distance. Using data from the MErcury Surface, Space ENvironment, GEochemistry, and Rangin…

2019 Journal of Geophysical Research (Space Physics)
VenusExpress 75
Two-Dimensional gcPIC Simulation of Rising-Tone Chorus Waves in a Dipole Magnetic Field
DOI: 10.1029/2019JA026586 Bibcode: 2019JGRA..124.4157L

Wang, Xueyi; Wang, Shui; Lu, Quanming +4 more

Rising-tone chorus waves have already been successfully produced in a mirror magnetic field with the use of one- and two-dimensional particle-in-cell (PIC) simulations. However, in reality, the background magnetic field in the inner Earth's magnetosphere is a dipole magnetic field, unlike symmetric mirror fields. In this paper, with the two-dimens…

2019 Journal of Geophysical Research (Space Physics)
Cluster 54
Universality of Lower Hybrid Waves at Earth's Magnetopause
DOI: 10.1029/2019JA027155 Bibcode: 2019JGRA..124.8727G

Lavraud, B.; Génot, V.; André, M. +15 more

Waves around the lower hybrid frequency are frequently observed at Earth's magnetopause and readily reach very large amplitudes. Determining the properties of lower hybrid waves is crucial because they are thought to contribute to electron and ion heating, cross-field particle diffusion, anomalous resistivity, and energy transfer between electrons…

2019 Journal of Geophysical Research (Space Physics)
Cluster 50
Global Empirical Picture of Magnetospheric Substorms Inferred From Multimission Magnetometer Data
DOI: 10.1029/2018JA025843 Bibcode: 2019JGRA..124.1085S

Sitnov, M. I.; Tsyganenko, N. A.; Stephens, G. K. +4 more

Magnetospheric substorms represent key explosive processes in the interaction of the Earth's magnetosphere with the solar wind, and their understanding and modeling are critical for space weather forecasting. During substorms, the magnetic field on the nightside is first stretched in the antisunward direction and then it rapidly contracts earthwar…

2019 Journal of Geophysical Research (Space Physics)
Cluster 48
MAVEN and MEX Multi-instrument Study of the Dayside of the Martian Induced Magnetospheric Structure Revealed by Pressure Analyses
DOI: 10.1029/2019JA026954 Bibcode: 2019JGRA..124.8564H

André, N.; Fedorov, A.; Barabash, S. +9 more

A combination of statistical studies and 18 case studies have been used to investigate the structure of the induced Martian magnetosphere. The different plasma and magnetic pressure forces on the dayside of the induced magnetosphere of Mars have been studied using 3.5 years of Mars Atmosphere and Volatile Evolution (MAVEN) and Mars Express (MEX) o…

2019 Journal of Geophysical Research (Space Physics)
MEx 45
SWAN/SOHO Lyman-α Mapping: The Hydrogen Geocorona Extends Well Beyond the Moon
DOI: 10.1029/2018JA026136 Bibcode: 2019JGRA..124..861B

Schmidt, W.; Bertaux, J. -L.; Quémerais, E. +2 more

The Earth's hydrogen exosphere Lyman-α radiation was mapped with the Solar Wind Anisotropies/Solar and Heliospheric Observatory (SWAN/SOHO) instrument in January 1996, 1997, and 1998 (low solar activity). The use of a hydrogen absorption cell allowed to disentangle the interplanetary emission from the geocoronal one and to assign the absorbed sign…

2019 Journal of Geophysical Research (Space Physics)
SOHO 38
Origin of the Extended Mars Radar Blackout of September 2017
DOI: 10.1029/2018JA026403 Bibcode: 2019JGRA..124.4556S

Leblanc, François; Witasse, Olivier; Sánchez-Cano, Beatriz +13 more

The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) onboard Mars Express, which operates between 0.1 and 5.5 MHz, suffered from a complete blackout for 10 days in September 2017 when observing on the nightside (a rare occurrence). Moreover, the Shallow Radar (SHARAD) onboard the Mars Reconnaissance Orbiter, which operates at 20…

2019 Journal of Geophysical Research (Space Physics)
MEx 38
The Martian Bow Shock Over Solar Cycle 23-24 as Observed by the Mars Express Mission
DOI: 10.1029/2018JA026404 Bibcode: 2019JGRA..124.4761H

Holmström, M.; Wild, J. A.; Lester, M. +2 more

The Martian bow shock position is known to be correlated with solar extreme ultraviolet irradiance. Since this parameter is also correlated with the evolution of the solar cycle, it is expected that the Martian bow shock position should also vary over such a period. However, previous reports on this topic have often proved contradictory. Using 13 …

2019 Journal of Geophysical Research (Space Physics)
MEx 37
Nighttime Magnetic Perturbation Events Observed in Arctic Canada: 2. Multiple-Instrument Observations
DOI: 10.1029/2019JA026797 Bibcode: 2019JGRA..124.7459E

Russell, C. T.; Kistler, L. M.; Fazakerley, A. +14 more

The rapid changes of magnetic fields associated with nighttime magnetic perturbations with amplitudes |ΔB| of hundreds of nanoteslas and 5- to 10-min periods can induce bursts of geomagnetically induced currents that can harm technological systems. This paper presents three cases of intervals of intense and complex nighttime magnetic perturbations…

2019 Journal of Geophysical Research (Space Physics)
Cluster 36
Signatures of Nonideal Plasma Evolution During Substorms Obtained by Mining Multimission Magnetometer Data
DOI: 10.1029/2019JA027037 Bibcode: 2019JGRA..124.8427S

Merkin, V. G.; Sitnov, M. I.; Genestreti, K. J. +5 more

Substorm-type evolution of the Earth's magnetosphere is investigated by mining more than two decades (1995-2017) of spaceborne magnetometer data from multiple missions including the first two years (2016-2017) of the Magnetospheric MultiScale mission. This investigation reveals interesting features of plasma evolution distinct from ideal magnetohy…

2019 Journal of Geophysical Research (Space Physics)
Cluster 35