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Mars' Ionopause: A Matter of Pressures
DOI: 10.1029/2020JA028145 Bibcode: 2020JGRA..12528145S

Holmstrom, Mats; Sánchez-Cano, Beatriz; Mayyasi, Majd +8 more

This study assesses under what circumstances the Martian ionopause is formed on the dayside, both in regions where there are strong crustal magnetic fields and areas where these fields are small (<30 nT). Multiple data sets from three MAVEN dayside deep dip campaigns are utilized between periapsis and 600-1,000 km, as well as solar wind observa…

2020 Journal of Geophysical Research (Space Physics)
MEx 48
Evolution of a Long-Duration Coronal Mass Ejection and Its Sheath Region Between Mercury and Earth on 9-14 July 2013
DOI: 10.1029/2019JA027213 Bibcode: 2020JGRA..12527213L

Farrugia, C. J.; Lugaz, N.; Winslow, R. M.

Using in situ measurements and remote-sensing observations, we study a coronal mass ejection (CME) that left the Sun on 9 July 2013 and impacted both Mercury and Earth while the planets were in radial alignment (within 3∘). The CME had an initial speed as measured by coronagraphs of 580 ± 20 km/s, an inferred speed at Mercury of 580 ± 30 km/s, and…

2020 Journal of Geophysical Research (Space Physics)
SOHO 37
20 Years of ACE Data: How Superposed Epoch Analyses Reveal Generic Features in Interplanetary CME Profiles
DOI: 10.1029/2020JA028150 Bibcode: 2020JGRA..12528150R

Auchère, F.; Démoulin, P.; Dasso, S. +4 more

Interplanetary coronal mass ejections (ICMEs) are magnetic structures propagating from the Sun's corona to the interplanetary medium. With over 20 years of observations at the L1 libration point, ACE offers hundreds of ICMEs detected at different times during several solar cycles and with different features such as the propagation speed. We invest…

2020 Journal of Geophysical Research (Space Physics)
SOHO 37
Magnetic Reconnection Inside a Flux Rope Induced by Kelvin-Helmholtz Vortices
DOI: 10.1029/2019JA027665 Bibcode: 2020JGRA..12527665H

Liu, Y.; Russell, C. T.; Escoubet, C. P. +23 more

On 5 May 2017, MMS observed a crater-type flux rope on the dawnside tailward magnetopause with fluctuations. The boundary-normal analysis shows that the fluctuations can be attributed to nonlinear Kelvin-Helmholtz (KH) waves. Reconnection signatures such as flow reversals and Joule dissipation were identified at the leading and trailing edges of t…

2020 Journal of Geophysical Research (Space Physics)
Cluster 35
The Influence of Spacecraft Charging on Low-Energy Ion Measurements Made by RPC-ICA on Rosetta
DOI: 10.1029/2019JA027478 Bibcode: 2020JGRA..12527478B

Stenberg Wieser, Gabriella; Wieser, Martin; Eriksson, Anders +2 more

Spacecraft charging is problematic for low-energy plasma measurements. The charged particles are attracted to or repelled from the charged spacecraft, affecting both the energy and direction of travel of the particles. The Ion Composition Analyzer (RPC-ICA) on board the Rosetta spacecraft is suffering from this effect. RPC-ICA was measuring positi…

2020 Journal of Geophysical Research (Space Physics)
Rosetta 33
Reconnection- and Dipolarization-Driven Auroral Dawn Storms and Injections
DOI: 10.1029/2019JA027663 Bibcode: 2020JGRA..12527663Y

Bonfond, B.; Vogt, M. F.; Mauk, B. H. +8 more

Jupiter displays many distinct auroral structures, among which auroral dawn storms and auroral injections are often observed contemporaneously. However, it is unclear if the contemporaneous nature of the observations is a coincidence or part of an underlying physical connection. We show six clear examples from a recent Hubble Space Telescope campa…

2020 Journal of Geophysical Research (Space Physics)
eHST 31
Do Statistical Models Capture the Dynamics of the Magnetopause During Sudden Magnetospheric Compressions?
DOI: 10.1029/2019JA027289 Bibcode: 2020JGRA..12527289S

Wild, J. A.; Milan, S. E.; Imber, S. M. +9 more

Under periods of strong solar wind driving, the magnetopause can become compressed, playing a significant role in draining electrons from the outer radiation belt. Also termed "magnetopause shadowing," this loss process has traditionally been attributed to a combination of magnetospheric compression and outward radial diffusion of electrons. Howev…

2020 Journal of Geophysical Research (Space Physics)
Cluster 29
Electron Pitch-Angle Distribution in Earth's Magnetotail: Pancake, Cigar, Isotropy, Butterfly, and Rolling-Pin
DOI: 10.1029/2020JA027777 Bibcode: 2020JGRA..12527777L

Wang, Z.; Xu, Y.; Chen, G. +4 more

Electron pitch-angle distributions, including isotropy, pancake, cigar, butterfly, and recently discovered rolling-pin distributions, are crucial to understanding electron dynamics in the magnetotail. However, occurrence rates of these distributions remain unclear. Here, for the first time, we reveal the occurrence rates of these distributions in …

2020 Journal of Geophysical Research (Space Physics)
Cluster 26
Effects of Fluctuating Magnetic Field on the Growth of the Kelvin-Helmholtz Instability at the Earth's Magnetopause
DOI: 10.1029/2019JA027515 Bibcode: 2020JGRA..12527515N

Hasegawa, H.; Nakamura, R.; Narita, Y. +5 more

At the Earth's magnetopause, the Kelvin-Helmholtz (KH) instability, driven by the persistent velocity shear between the magnetosheath and the magnetosphere, has been frequently observed during northward interplanetary magnetic field periods and considered as one of the most important candidates for transporting and mixing plasmas across the magnet…

2020 Journal of Geophysical Research (Space Physics)
Cluster 22
Comparisons Between Jupiter's X-ray, UV and Radio Emissions and In-Situ Solar Wind Measurements During 2007
DOI: 10.1029/2019JA027222 Bibcode: 2020JGRA..12527222D

Jackman, C. M.; Lamy, L.; Branduardi-Raymont, G. +21 more

We compare Chandra and XMM-Newton X-ray observations of Jupiter during 2007 with a rich multi-instrument data set including upstream in situ solar wind measurements from the New Horizons spacecraft, radio emissions from the Nançay Decametric Array and Wind/Waves, and ultraviolet (UV) observations from the Hubble Space Telescope. New Horizons data …

2020 Journal of Geophysical Research (Space Physics)
eHST 21