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Terrestrial OH nightglow measurements during the Rosetta flyby
DOI: 10.1002/2015GL064485 Bibcode: 2015GeoRL..42.5670M

Piccioni, G.; Capaccioni, F.; Soret, L. +5 more

We present a study of the terrestrial hydroxyl nightglow emissions observed with the Visible and Infrared Thermal Imaging Spectrometer on board the Rosetta mission. During these observations, the OH Δv = 1 and 2 sequences were measured simultaneously. This allowed investigating the relative population of the v = 1 to 9 vibrational levels by using …

2015 Geophysical Research Letters
Rosetta 5
The energy-based scaling of a thin current sheet: Case study
DOI: 10.1002/2015GL066189 Bibcode: 2015GeoRL..42.9609S

Sasunov, Yu. L.; Khodachenko, M. L.; Alexeev, I. I. +3 more

The influence of average plasma energy on the half thickness ℓ of a thin current sheet (TCS) is investigated for three cases of TCSs crossings. The value of ℓ was estimated from the magnetic field data by means of Cluster observations. The obtained scaling values for TCSs, , where ρT is the thermal Larmor radius, were compared with the …

2015 Geophysical Research Letters
Cluster 2
Anomalous expansion of coronal mass ejections during solar cycle 24 and its space weather implications
DOI: 10.1002/2014GL059858 Bibcode: 2014GeoRL..41.2673G

Gopalswamy, Nat; Akiyama, Sachiko; Yashiro, Seiji +3 more

The familiar correlation between the speed and angular width of coronal mass ejections (CMEs) is also found in solar cycle 24, but the regression line has a larger slope: for a given CME speed, cycle 24 CMEs are significantly wider than those in cycle 23. The slope change indicates a significant change in the physical state of the heliosphere, due…

2014 Geophysical Research Letters
SOHO 134
Unexpected variability of Martian hydrogen escape
DOI: 10.1002/2013GL058578 Bibcode: 2014GeoRL..41..314C

Montmessin, Franck; Bertaux, Jean-Loup; Chaffin, Michael S. +3 more

Mars today is much drier than the Earth, though they likely began with similar relative amounts of water. One potential cause for this discrepancy is hydrogen loss to space, which may have removed a large fraction of Mars' initial water. Here we demonstrate an order-of-magnitude change in the Martian hydrogen escape rate in 2007, inconsistent with…

2014 Geophysical Research Letters
MEx 133
The bathymetry of a Titan sea
DOI: 10.1002/2013GL058618 Bibcode: 2014GeoRL..41.1432M

Paillou, Philippe; Zebker, Howard; Lunine, Jonathan +9 more

We construct the depth profile—the bathymetry—of Titan's large sea Ligeia Mare from Cassini RADAR data collected during the 23 May 2013 (T91) nadir-looking altimetry flyby. We find the greatest depth to be about 160 m and a seabed slope that is gentler toward the northern shore, consistent with previously imaged shoreline morphologies. Low radio s…

2014 Geophysical Research Letters
Cassini 124
A rapid decrease of the hydrogen corona of Mars
DOI: 10.1002/2014GL061803 Bibcode: 2014GeoRL..41.8013C

Quemerais, E.; Bertaux, J. -L.; Chaufray, J. -Y. +4 more

Mars is believed to have lost much of its surface water 3.5 billion years ago, but the amounts that escaped into space and remain frozen in the crust today are not well known. Hydrogen atoms in the extended martian atmosphere, some of which escape the planet's gravity, can be imaged through scattered solar UV radiation. Hubble Space Telescope (HST…

2014 Geophysical Research Letters
eHST 93
Propagation of lower-band whistler-mode waves in the outer Van Allen belt: Systematic analysis of 11 years of multi-component data from the Cluster spacecraft
DOI: 10.1002/2014GL059815 Bibcode: 2014GeoRL..41.2729S

Santolík, Ondřej; Cornilleau-Wehrlin, Nicole; Kolmašová, Ivana +2 more

Lower-band whistler-mode emissions can influence the dynamics of the outer Van Allen radiation belts. We use 11 years of measurements of the STAFF-SA instruments onboard the four Cluster spacecraft to systematically build maps of wave propagation parameters as a function of position. We determine probability distributions of wave vector angle weig…

2014 Geophysical Research Letters
Cluster 78
Wave activities in separatrix regions of magnetic reconnection
DOI: 10.1002/2014GL059893 Bibcode: 2014GeoRL..41.2721F

Fujimoto, Keizo

Two-dimensional particle-in-cell simulations have reproduced the waves consistent with those observed frequently in the separatrix regions of magnetic reconnection in the Earth's magnetotail. The key process generating the waves is intense parallel acceleration of the electrons due to an electrostatic potential hump formed in the inflow side of th…

2014 Geophysical Research Letters
Cluster 78
First observation of rising-tone magnetosonic waves
DOI: 10.1002/2014GL061867 Bibcode: 2014GeoRL..41.7419F

Santolík, O.; Chen, L.; Cao, J. B. +7 more

Magnetosonic (MS) waves are linearly polarized emissions confined near the magnetic equator with wave normal angle near 90° and frequency below the lower hybrid frequency. Such waves, also termed equatorial noise, were traditionally known to be "temporally continuous" in their time-frequency spectrogram. Here we show for the first time that MS wav…

2014 Geophysical Research Letters
Cluster 69
Cold electron heating by EMIC waves in the plasmaspheric plume with observations of the Cluster satellite
DOI: 10.1002/2014GL059241 Bibcode: 2014GeoRL..41.1830Y

Dandouras, Iannis; Yuan, Zhigang; Huang, Shiyong +7 more

We report in situ observations by the Cluster spacecraft of plasmaspheric electron heating in the plasmaspheric plume. Electron heating events were accompanied by enhancements of electromagnetic ion cyclotron (EMIC) waves in the increased density ducts on the negative density gradient side for two substructures of the plasmaspheric plume. Electron…

2014 Geophysical Research Letters
Cluster 60