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Intense plasma wave emissions associated with Saturn's moon Rhea
DOI: 10.1029/2011GL049219 Bibcode: 2011GeoRL..3819204S

Schippers, P.; Gurnett, D. A.; Russell, C. T. +7 more

Measurements by the Cassini spacecraft during a close flyby of Saturn's moon Rhea on March 2, 2010, show the presence of intense plasma waves in the magnetic flux tube connected to the surface of the moon. Three types of waves were observed, (1) bursty electrostatic waves near the electron plasma frequency, (2) intense whistler-mode emissions belo…

2011 Geophysical Research Letters
Cassini 33
Scattering function for energetic neutral hydrogen atoms off the lunar surface
DOI: 10.1029/2011GL049362 Bibcode: 2011GeoRL..3822202S

Barabash, S.; Holmström, M.; Futaana, Y. +7 more

The Sub-keV Atom Reflecting Analyzer instrument on board the lunar orbiter Chandrayaan-1 provided a large number of measurements of lunar energetic neutral atoms (ENAs). These ENAs were formerly solar wind ions, which were neutralized and backscattered from the lunar surface. The angles under which the ENAs are scattered strongly depend on the sol…

2011 Geophysical Research Letters
Chandrayaan-1 32
Low-altitude acceleration of ionospheric ions at Mars
DOI: 10.1029/2011GL047064 Bibcode: 2011GeoRL..38.8108L

Barabash, S.; Lundin, R.; Yamauchi, M. +2 more

The objective of this study is to understand the acceleration processes that lead to outflow and escape of ionospheric ions from Mars. Observations show that accelerated dayside and flank ionospheric ions move slowly antisunward along the direction of the external/magnetosheath flow. At high altitudes, in the central tail, ions are further acceler…

2011 Geophysical Research Letters
MEx 31
Large-amplitude whistler waves and electron acceleration
DOI: 10.1029/2011GL047893 Bibcode: 2011GeoRL..3812105Y

Yoon, Peter H.

A recent observation shows that large-amplitude whistler waves propagating obliquely with respect to the ambient magnetic field may be responsible for energizing the radiation belt electrons to relativistic energies (MeV) within a time scale as short as a fraction of a second. Test-particle simulations available in the literature invariably adopt …

2011 Geophysical Research Letters
Cluster 31
Cluster observations of whistler mode ducts and banded chorus
DOI: 10.1029/2011GL049112 Bibcode: 2011GeoRL..3818107H

Pickett, J. S.; Facskó, G.; Inan, U. S. +3 more

Bell et al. (2009) proposed that the source region for banded chorus consists of whistler mode ducts of depleted electron density (Ne) for upper band (UB) chorus for all wave normal angles ($\theta$) and ducts of either enhanced or depleted Ne for lower band (LB) chorus for small $\theta$ and $\theta$ near or greater than the…

2011 Geophysical Research Letters
Cluster 29
Electromagnetic ion cyclotron waves in the helium branch induced by multiple electromagnetic ion cyclotron triggered emissions
DOI: 10.1029/2011GL048427 Bibcode: 2011GeoRL..3817102S

Dandouras, Iannis; Omura, Yoshiharu; Shoji, Masafumi +3 more

Electromagnetic ion cyclotron (EMIC) triggered emissions with rising tones between the H+ and He+ cyclotron frequencies were found in the inner magnetosphere by the recent Cluster observations. Another type of EMIC wave with a constant frequency is occasionally observed below the He+ cyclotron frequency after the m…

2011 Geophysical Research Letters
Cluster 29
Location of Saturn's northern infrared aurora determined from Cassini VIMS images
DOI: 10.1029/2010GL046193 Bibcode: 2011GeoRL..38.3102B

Brown, R. H.; Baines, K. H.; Dougherty, M. K. +6 more

The location of Saturn's northern infrared aurora is described in detail using 12 selected images acquired by Cassini VIMS during 2006-2008. Bright main oval arcs and prevalent polar features are displayed, which do not exhibit a preferred local time or spatial extent. The average equatorward limit of the aurora was determined using a best fit cir…

2011 Geophysical Research Letters
Cassini 28
Magnetic signatures of a tenuous atmosphere at Dione
DOI: 10.1029/2011GL048454 Bibcode: 2011GeoRL..3815102S

Dougherty, Michele K.; Saur, Joachim; Simon, Sven +2 more

We present Cassini magnetic field observations from the only two close flybys (16DI and 129DI) of Saturn's icy satellite Dione which have been carried out so far. Data from 16DI show a weak field perturbation in the upstream region, indicative of a tenuous atmosphere around the satellite. By applying an analytical model of the perturbations caused…

2011 Geophysical Research Letters
Cassini 26
Resolution of the lunar hydrogen enigma
DOI: 10.1029/2011GL046688 Bibcode: 2011GeoRL..38.6201H

Hodges, R. R.

The recent discovery, by instruments on the IBEX and Chandrayaan-1 spacecraft, of significant fluxes of energetic hydrogen atoms escaping from the moon suggests that there are flaws in the common wisdom regarding the interaction of solar wind with lunar regolith that have prevailed in attempts to explain the failure of the Apollo 17 far-ultraviole…

2011 Geophysical Research Letters
Chandrayaan-1 25
Hot electrons as tracers of large-scale structure of magnetotail current sheets
DOI: 10.1029/2011GL047979 Bibcode: 2011GeoRL..3814102A

Petrukovich, A. A.; Zelenyi, L. M.; Nakamura, R. +1 more

This paper is devoted to the investigation of the vertical electron temperature distribution in thin currents sheets of the Earth magnetotail. The dependence of electron temperature on magnetic field Te(Bx) is examined for 62 thin currents sheet crossings by the Cluster spacecraft. The profiles Te(Bx) ar…

2011 Geophysical Research Letters
Cluster 25