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ENA periodicities and their phase relations to SKR emissions at Saturn
DOI: 10.1029/2011GL048418 Bibcode: 2011GeoRL..3816106C

Gurnett, D. A.; Krimigis, S. M.; Mitchell, D. G. +2 more

Cassini orbits during days 200-366 in 2004 afforded the opportunity to continuously observe energetic neutral atom (ENA) emissions from long range (>50 RS, 1 RS = 60268 km) on Saturn's dawn side. Images of energetic neutral hydrogen (25-55 keV) and oxygen (90-160 keV) were projected onto the noon-midnight plane, corrected …

2011 Geophysical Research Letters
Cassini 7
Cassini magnetometer observations over the Enceladus poles
DOI: 10.1029/2011GL049013 Bibcode: 2011GeoRL..3819109J

Persoon, A. M.; Russell, C. T.; Wei, H. Y. +5 more

In 2009 and 2010, the Cassini spacecraft made seven targeted Enceladus flybys along trajectories parallel to the equatorial plane. The magnetometer on board Cassini made a complete set of vector field distribution measurements on these tracks and observed significant perturbations that further constrained the location of the momentum-exchange regi…

2011 Geophysical Research Letters
Cassini 6
Conjunction of anti-parallel and component reconnection at the dayside MP: Cluster and Double Star coordinated observation on 6 April 2004
DOI: 10.1029/2011GL047125 Bibcode: 2011GeoRL..3810105W

Wei, Y.; Dunlop, M. W.; Bogdanova, Y. V. +7 more

Previous theoretical and simulation studies have suggested that the anti-parallel and component reconnection can occur simultaneously on the dayside magnetopause. Certain observations have also been reported to support global conjunct pattern of magnetic reconnection. Here, we show direct evidence for the conjunction of anti-parallel and component…

2011 Geophysical Research Letters
Cluster DoubleStar 3
Tidal variations in the Martian lower atmosphere inferred from Mars Express Planetary Fourier Spectrometer temperature data
DOI: 10.1029/2011GL050348 Bibcode: 2011GeoRL..3824205S

Grassi, D.; Kasaba, Y.; Formisano, V. +4 more

We report on the characteristics of tidal variations in the Martian lower atmosphere (<45 km) using the Mars Express (MEX) Planetary Fourier Spectrometer (PFS) temperature data for about three Martian years (between the ends of MY26 and MY29). The PFS data, which widely cover local time, enable us to investigate diurnal variations in the atmosp…

2011 Geophysical Research Letters
MEx 2
Correction to “Are the basins of Titan's Hotei Regio and Tui Regio sites of former low latitude seas?”
DOI: 10.1029/2011GL046753 Bibcode: 2011GeoRL..38.4201M

Moore, Jeffrey M.; Howard, Alan D.

Abstract Available from http://www.agu.org

2011 Geophysical Research Letters
Cassini 2