Search Publications

Direct evidence of differences in magnetic rotation rate between Saturn's northern and southern polar regions
DOI: 10.1029/2010JA016070 Bibcode: 2011JGRA..116.1201S

Southwood, David

The discovery of a difference in apparent rotation rate between Saturn kilometric radio emission from northern and southern hemispheres leads immediately to the question of whether there is a counterpart detectable in the Saturnian magnetic field. We report direct detection of a difference in the rotating magnetic signal measured by the Cassini sp…

2011 Journal of Geophysical Research (Space Physics)
Cassini 34
Pitch angle evolutions of oxygen ions driven by storm time ULF poloidal standing waves
DOI: 10.1029/2010JA016047 Bibcode: 2011JGRA..116.3207Y

Zong, Q. -G.; Reme, H.; Fu, S. Y. +9 more

We present the first systematic observational study on the pitch angle evolutions of O+ ions associated with ULF Pc5 poloidal standing waves excited during geomagnetic storms. The O+ ion measurements are made on board the CLUSTER satellites with the Composition Distribution Function (CODIF) instrument, which covers energies f…

2011 Journal of Geophysical Research (Space Physics)
Cluster 33
Transient Pc3 wave activity generated by a hot flow anomaly: Cluster, Rosetta, and ground-based observations
DOI: 10.1029/2011JA016467 Bibcode: 2011JGRA..116.8224E

Glassmeier, K. -H.; Eastwood, J. P.; Wild, J. A. +6 more

Pc3 pulsations are observed in the magnetosphere with wave periods of 10-45 s. Two distinct populations have been observed; one exhibits a frequency dependence on the solar wind magnetic field strength, whereas the other does not. The first population is explained in terms of a model where the bow shock reflects ions which generate upstream foresh…

2011 Journal of Geophysical Research (Space Physics)
Cluster Rosetta 32
Multispacecraft observations of chorus emissions as a tool for the plasma density fluctuations' remote sensing
DOI: 10.1029/2011JA016540 Bibcode: 2011JGRA..116.9222A

Khotyaintsev, Yuri; Dudok de Wit, Thierry; Agapitov, Oleksiy +4 more

Discrete ELF/VLF chorus emissions are the most intense electromagnetic plasma waves that are observed in the radiation belts and in the outer magnetosphere of the Earth. They are assumed to propagate approximately along the magnetic field lines and are generated in source regions in the vicinity of the magnetic equator and in minimum B pockets in …

2011 Journal of Geophysical Research (Space Physics)
Cluster 32
Locations of boundaries of outer and inner radiation belts as observed by Cluster and Double Star
DOI: 10.1029/2010JA016376 Bibcode: 2011JGRA..116.9234G

Dandouras, I.; Cao, J.; Ganushkina, N. Yu +1 more

Cluster CIS ion spectrograms measured during the period of the recent solar minimum between April 2007 and June 2009, when Cluster was deep in the radiation belts with its perigee as close as L = 2, are analyzed. The analysis is complemented by Double Star TC-1 satellite data from HIA ion spectrograms on perigee passes during the period of May 15,…

2011 Journal of Geophysical Research (Space Physics)
Cluster DoubleStar 32
The relations between magnetospheric chorus and hiss inside and outside the plasmasphere boundary layer: Cluster observation
DOI: 10.1029/2010JA016240 Bibcode: 2011JGRA..116.7221W

Zong, Qiugang; Xiao, Fuliang; Wang, Yongfu +3 more

Magnetospheric whistler mode emissions (chorus and hiss) can play an important role in acceleration and loss of energetic electrons by wave-particle interaction. Here we present a first report of two events in the simultaneous observations of chorus and hiss by the Cluster constellation. During the event of 30 August 2001, one spacecraft observed …

2011 Journal of Geophysical Research (Space Physics)
Cluster 32
The influence of pickup protons, from interstellar neutral hydrogen, on the propagation of interplanetary shocks from the Halloween 2003 solar events to ACE and Ulysses: A 3-D MHD modeling study
DOI: 10.1029/2010JA015803 Bibcode: 2011JGRA..116.3105D

Dryer, M.; Sun, W.; Intriligator, D. S. +3 more

We describe our 3-D, time-dependent, MHD solar wind model that we recently modified to include the physics of pickup protons from interstellar neutral hydrogen. The model has a time-dependent lower boundary condition, at 0.1 AU, that is driven by source surface map files through an empirical interface module. We describe the empirical interface an…

2011 Journal of Geophysical Research (Space Physics)
Ulysses 31
Analysis of Saturn kilometric radiation near a source center
DOI: 10.1029/2011JA017056 Bibcode: 2011JGRA..11612222M

Schippers, P.; Gurnett, D. A.; Lamy, L. +3 more

The Cassini spacecraft flew very near a source region of Saturn kilometric radiation (SKR) on day 73 of 2008, the second known encounter with a source region at high latitude. The radio and plasma wave instrument, Radio and Plasma Wave Science, observed intense kilometric emission in the extraordinary X mode, ordinary O mode, and Z mode. The elect…

2011 Journal of Geophysical Research (Space Physics)
Cassini 31
Statistical characteristics of field-aligned currents in Saturn's nightside magnetosphere
DOI: 10.1029/2010JA016102 Bibcode: 2011JGRA..116.4213T

Coates, A. J.; Dougherty, M. K.; Cowley, S. W. H. +3 more

During 2008, the Cassini spacecraft traversed Saturn's high-latitude field-aligned current systems on sequential north-south periapsis passes in the nightside magnetosphere. Two types of current systems have previously been identified, associated with antisymmetric azimuthal field signatures in the northern and southern hemispheres. The first exhi…

2011 Journal of Geophysical Research (Space Physics)
Cassini 30
Stream particles as the probe of the dust-plasma-magnetosphere interaction at Saturn
DOI: 10.1029/2011JA016488 Bibcode: 2011JGRA..116.9215H

Kempf, S.; Postberg, F.; Srama, R. +5 more

We analyze the dynamics and composition of Saturnian stream particles measured by the Cosmic Dust Analyser (CDA) onboard the Cassini spacecraft. To reconstruct the dynamical properties of Saturnian stream particles, we adopt a backward tracing method with in situ solar wind measurements to filter out the influence of the interplanetary magnetic fi…

2011 Journal of Geophysical Research (Space Physics)
Cassini 30