Search Publications

Cassini VIMS observations of H3+ emission on the nightside of Jupiter
DOI: 10.1002/2015JA021097 Bibcode: 2015JGRA..120.6948S

Baines, Kevin H.; Brown, Robert H.; O'Donoghue, James +10 more

We present the first detailed analysis of H3+ nightside emission from Jupiter, using Visual and Infrared Mapping Spectrometer (VIMS) data from the Cassini flyby in 2000-2001, producing the first Jovian maps of nightside H3+ emission, temperature, and column density. Using these, we identify and character…

2015 Journal of Geophysical Research (Space Physics)
Cassini 16
The ULF wave foreshock boundary: Cluster observations
DOI: 10.1002/2014JA020783 Bibcode: 2015JGRA..120.4181A

Mazelle, Christian; Andrés, Nahuel; Meziane, Karim +2 more

The interaction of backstreaming ions with the incoming solar wind in the upstream region of the bow shock gives rise to a number of plasma instabilities from which ultralow frequency (ULF) waves can grow. Because of their finite growth rate, the ULF waves are spatially localized in the foreshock region. Previous studies have reported observationa…

2015 Journal of Geophysical Research (Space Physics)
Cluster 16
Case and statistical studies on the evolution of hot flow anomalies
DOI: 10.1002/2014JA020862 Bibcode: 2015JGRA..120.6332Z

Zhao, L. L.; Zhang, H.; Wang, S. +1 more

Hot flow anomalies (HFAs) frequently observed near Earth's bow shock are phenomena resulting from the interaction between interplanetary discontinuities and Earth's bow shock. We identify 199 HFA events using Cluster data from 2001 to 2010 and divide these events into four categories according to the dynamic pressure profile, namely, "-+," "+-," "…

2015 Journal of Geophysical Research (Space Physics)
Cluster 16
A new stationary analytical model of the heliospheric current sheet and the plasma sheet
DOI: 10.1002/2015JA021294 Bibcode: 2015JGRA..120.8210K

Malova, Helmi V.; Kislov, Roman A.; Khabarova, Olga V.

We develop a single-fluid 2-D analytical model of the axially symmetric thin heliospheric current sheet (HCS) embedded into the heliospheric plasma sheet (HPS). A HCS-HPS system has a shape of a relatively thin plasma disk limited by separatrices that also represent current sheets, which is in agreement with Ulysses observations in the aphelion, w…

2015 Journal of Geophysical Research (Space Physics)
Ulysses 16
Estimation of cold plasma outflow during geomagnetic storms
DOI: 10.1002/2015JA021810 Bibcode: 2015JGRA..12010622H

André, M.; Eriksson, A.; Haaland, S. +11 more

Low-energy ions of ionospheric origin constitute a significant contributor to the magnetospheric plasma population. Measuring cold ions is difficult though. Observations have to be done at sufficiently high altitudes and typically in regions of space where spacecraft attain a positive charge due to solar illumination. Cold ions are therefore shiel…

2015 Journal of Geophysical Research (Space Physics)
Cluster 16
Sustained lobe reconnection in Saturn's magnetotail
DOI: 10.1002/2015JA021768 Bibcode: 2015JGRA..12010257T

Thomsen, M. F.; Jackman, C. M.; Kurth, W. S. +3 more

The degree to which solar wind driving may affect Saturn's magnetosphere is not yet fully understood. We present observations that suggest that under some conditions the solar wind does govern the character of the plasma sheet in Saturn's outer magnetosphere. On 16 September 2006, the Cassini spacecraft, at a radial distance of 37 Rs ne…

2015 Journal of Geophysical Research (Space Physics)
Cassini 16
The impact of a slow interplanetary coronal mass ejection on Venus
DOI: 10.1002/2014JA020616 Bibcode: 2015JGRA..120.3489C

Barabash, Stas; Futaana, Yoshifumi; Collinson, Glyn A. +8 more

We present Venus Express observations of the impact of a slow interplanetary coronal mass ejection (ICME), which struck Venus on 23 December 2006, creating unusual quasi steady state upstream conditions for the 2 h close to periapsis: an enhanced (∼ nT) interplanetary magnetic field (IMF), radially aligned with the Sun-Venus line; and a dense (∼ c…

2015 Journal of Geophysical Research (Space Physics)
VenusExpress 16
What is the nature of magnetosheath FTEs?
DOI: 10.1002/2015JA020983 Bibcode: 2015JGRA..120.4576R

Robert, Patrick; Louarn, Philippe; Fontaine, Dominique +3 more

Cluster multipoint measurements are used to study two successive magnetosheath flux transfer events (FTEs). Magnetic field lines in the leading region are found to be closed magnetospheric field lines. For event 1 these field lines are wounded up by a large current structure oriented eastward and moving poleward. Conversely, the trailing region co…

2015 Journal of Geophysical Research (Space Physics)
Cluster 16
Transpolar arc observation after solar wind entry into the high-latitude magnetosphere
DOI: 10.1002/2014JA020912 Bibcode: 2015JGRA..120.3525M

Wei, Y.; Zong, Q. -G.; Fear, R. C. +11 more

Recently, Cluster observations have revealed the presence of new regions of solar wind plasma entry at the high-latitude magnetospheric lobes tailward of the cusp region, mostly during periods of northward interplanetary magnetic field. In this study, observations from the Global Ultraviolet Imager (GUVI) experiment on board the TIMED spacecraft a…

2015 Journal of Geophysical Research (Space Physics)
Cluster 15
Fast damping of ultralow frequency waves excited by interplanetary shocks in the magnetosphere
DOI: 10.1002/2014JA020761 Bibcode: 2015JGRA..120.2438W

Zong, Qiugang; Rankin, Robert; Wang, Chengrui

Analysis of Cluster spacecraft data shows that intense ultralow frequency (ULF) waves in the inner magnetosphere can be excited by the impact of interplanetary shocks and solar wind dynamic pressure variations. The observations reveal that such waves can be damped away rapidly in a few tens of minutes. Here we examine mechanisms of ULF wave dampin…

2015 Journal of Geophysical Research (Space Physics)
Cluster 14