Search Publications

On the Edgeworth-Kuiper Belt dust flux to Saturn
DOI: 10.1029/2012GL052530 Bibcode: 2012GeoRL..3915104P

Horányi, Mihály; Poppe, Andrew R.

Dust grains originating from the Edgeworth-Kuiper Belt (EKB) are believed to be the dominant species of dust in the outer solar system. These grains, evolving inward from the EKB under the influence of a variety of forces, will encounter the giant planets or their ring and moon systems. At Saturn, this influx drives several physical processes incl…

2012 Geophysical Research Letters
Cassini 13
Titan airglow during eclipse
DOI: 10.1029/2012GL053230 Bibcode: 2012GeoRL..3918204W

Strobel, D. F.; West, R. A.; Gladstone, G. R. +4 more

Solar XUV photons can provide enough energy to account for the observed nitrogen UV dayglow emissions above 800 km, but a small or sporadic contribution from energetic particles cannot be ruled out. Furthermore, ion production at altitudes deeper than 800 km as inferred from radio occultation cannot be produced by solar XUV stimulation and implies…

2012 Geophysical Research Letters
Cassini 13
Accelerated magnetosheath flows caused by IMF draping: Dependence on latitude
DOI: 10.1029/2011GL050209 Bibcode: 2012GeoRL..39.1103E

Farrugia, C. J.; Erkaev, N. V.; Torbert, R. B. +2 more

In previous work we used a semi-analytical treatment to describe accelerated magnetosheath flows caused by the draping of interplanetary magnetic field (IMF) lines around the magnetosphere. Here, we use the same approach, i.e., modeling the magnetic field lines as elastic strings, to examine how the magnetic tension force, one of the two agents re…

2012 Geophysical Research Letters
Cluster 11
The observed composition of ions outflowing from Titan
DOI: 10.1029/2012GL053079 Bibcode: 2012GeoRL..3919104W

Luhmann, J. G.; Mitchell, D. G.; Wahlund, J. -E. +8 more

We report on Cassini Ion and Neutral Mass Spectrometer (INMS) observations above Titan's exobase at altitudes of 2225 km to 3034 km. We observe significant densities of CH5+, HCNH+ and C2H5+ that require ion-molecule reactions to be produced in the quantities observed. The measured …

2012 Geophysical Research Letters
Cassini 10
Spacecraft charging near Enceladus
DOI: 10.1029/2012GL050999 Bibcode: 2012GeoRL..39.6108H

Kempf, S.; Grün, E.; Hsu, H. -W. +1 more

In the vicinity of Enceladus, a geologically active moon of Saturn, the modeled spacecraft potential is significantly more negative than indicated by the Cassini Langmuir probe measurements. To understand this potential difference, we introduce two new dust-related charging currents: a) the dust ram current; and b) the dust impact-plasma current, …

2012 Geophysical Research Letters
Cassini 10
First observation of the Venus UV dayglow at limb from SPICAV/VEX
DOI: 10.1029/2012GL053626 Bibcode: 2012GeoRL..3920201C

Bertaux, Jean-Loup; Chaufray, Jean-Yves; Leblanc, Francois

We present the first limb observations of the dayglow emissions by the UV channel of SPICAV aboard Venus Express between October and December 2011. The CO Cameron bands between 180-260 nm and CO2+ doublet at 289 nm are clearly identified for the first time in the Venusian dayglow. The Cameron bands brightness peaks at 137.5 ±…

2012 Geophysical Research Letters
VenusExpress 8
Spatial dependence of banded chorus intensity near the magnetic equator
DOI: 10.1029/2012GL052929 Bibcode: 2012GeoRL..3917103H

Pickett, J. S.; Inan, U. S.; Bell, T. F. +1 more

Data from 12 different Cluster orbits containing banded chorus emissions, with observations from 22 different events spread across the four Cluster spacecraft, are used to show the spatial dependence of banded chorus intensity near the magnetic equator under conditions of moderate magnetic disturbance (Kp ≤ 5). The intensities for upper…

2012 Geophysical Research Letters
Cluster 7
Consequences of negative ions for Titan's plasma interaction
DOI: 10.1029/2012GL053835 Bibcode: 2012GeoRL..3920103L

Brecht, Stephen H.; Ledvina, Stephen A.

A hybrid particle code has been used to examine how Titan's interaction with Saturn's magnetosphere is affected by the presence of negative ions in Titan's ionosphere. The simulations self-consistently include a version of Titan's ionosphere represented by 8 generic positive ion species, over 40 ion-neutral chemical reactions, ion-neutral collisio…

2012 Geophysical Research Letters
Cassini 7
Magnetospheric line radiation event observed simultaneously on board Cluster 1, Cluster 2 and DEMETER spacecraft
DOI: 10.1029/2012GL053132 Bibcode: 2012GeoRL..3918103N

Pickett, J. S.; Santolík, O.; Parrot, M. +1 more

We present a case study of a magnetospheric line radiation (MLR) event observed simultaneously by Cluster 1 and Cluster 2 during a perigee passage at a radial distance of about 4 RE and, at the same time, by the low-orbiting DEMETER satellite. This unique constellation enables us to analyze spatiotemporal variability of the phenomenon. …

2012 Geophysical Research Letters
Cluster 7
Cassini capturing of freshly-produced water-group ions in the Enceladus torus
DOI: 10.1029/2012GL053173 Bibcode: 2012GeoRL..3918108Y

Yaroshenko, V. V.; Miloch, W. J.; Thomas, H. M. +1 more

The water vapor plume on the geological-active south-polar region of the moon Enceladus is recognized as the main source of Saturn's neutral torus centered on the Enceladus orbit. The composition of the torus is dominated by water group species. Recent in situ Cassini plasma spectrometer measurements indicate the existence of freshly produced, slo…

2012 Geophysical Research Letters
Cassini 6