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Goniopolarimetric study of the revolution 29 perikrone using the Cassini Radio and Plasma Wave Science instrument high-frequency radio receiver
DOI: 10.1029/2008JA013830 Bibcode: 2009JGRA..114.3215C

Kurth, W. S.; Cecconi, B.; Lamy, L. +3 more

We present goniopolarimetric (also known as direction finding) results of the Saturn kilometric radiation (SKR), using the Cassini Radio and Plasma Wave Science instrument high-frequency radio receiver data. Tools to retrieve the characteristics of the SKR sources have been developed that allow us to measure their 3-D location and beaming angle re…

2009 Journal of Geophysical Research (Space Physics)
Cassini 63
On the character and distribution of lower-frequency radio emissions at Saturn and their relationship to substorm-like events
DOI: 10.1029/2008JA013997 Bibcode: 2009JGRA..114.8211J

Dougherty, M. K.; Jackman, C. M.; Kurth, W. S. +5 more

With the arrival of the Cassini spacecraft at Saturn in July 2004, there have been quasi-continuous observations of Saturn kilometric radiation (SKR) emissions. Exploration of the nightside magnetosphere has revealed evidence of plasmoid-like magnetic structures and other phenomena indicative of the Kronian equivalent of terrestrial substorms. In …

2009 Journal of Geophysical Research (Space Physics)
Cassini 62
Multispacecraft recovery of a magnetic cloud and its origin from magnetic reconnection on the Sun
DOI: 10.1029/2008JA013657 Bibcode: 2009JGRA..114.4102M

Luhmann, J. G.; Möstl, C.; Farrugia, C. J. +8 more

Multipoint spacecraft observations of a magnetic cloud on 22 May 2007 have given us the opportunity to apply a multispacecraft technique to infer the structure of this large-scale magnetic flux rope in the solar wind. Combining WIND and STEREO-B magnetic field and plasma measurements, we construct a combined magnetic field map by integrating the G…

2009 Journal of Geophysical Research (Space Physics)
SOHO 62
Foreshock compressional boundary
DOI: 10.1029/2008JA013950 Bibcode: 2009JGRA..114.8205O

Omidi, N.; Blanco-Cano, X.; Sibeck, D. G.

We employ 2.5-D electromagnetic, hybrid simulations that treat ions kinetically via particle-in-cell methods and electrons as a massless fluid to study the formation and properties of a newly discovered boundary named the foreshock compressional boundary (FCB). This boundary forms in the ion foreshock and is associated with enhanced densities and …

2009 Journal of Geophysical Research (Space Physics)
Cluster 60
Diurnal variations of Titan's ionosphere
DOI: 10.1029/2009JA014228 Bibcode: 2009JGRA..114.6310C

Wahlund, J. -E.; Galand, M.; Waite, J. H. +7 more

We present our analysis of the diurnal variations of Titan's ionosphere (between 1000 and 1300 km) based on a sample of Ion Neutral Mass Spectrometer (INMS) measurements in the Open Source Ion (OSI) mode obtained from eight close encounters of the Cassini spacecraft with Titan. Although there is an overall ion depletion well beyond the terminator,…

2009 Journal of Geophysical Research (Space Physics)
Cassini 57
A mechanism for electrostatic solitary structures in the Earth's magnetosheath
DOI: 10.1029/2009JA014306 Bibcode: 2009JGRA..114.9212L

Lakhina, G. S.; Pickett, J. S.; ViñAs, A. F. +3 more

Electrostatic solitary waves (ESWs) have been observed in the Earth's magnetosheath region by Cluster. A mechanism for the generation of these structures in terms of electron-acoustic solitons and double layers is discussed. The model simulates the magnetosheath plasma by a four-component plasma system consisting of core electrons, two counterstre…

2009 Journal of Geophysical Research (Space Physics)
Cluster 56
Steep, transient density gradients in the Martian ionosphere similar to the ionopause at Venus
DOI: 10.1029/2009JA014711 Bibcode: 2009JGRA..11412310D

Gurnett, D. A.; Winningham, J. D.; Frahm, R. A. +3 more

With the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) on the Mars Express (MEX) spacecraft, the electron density can be measured by two methods: from the excitation of local plasma oscillations and from remote sounding. A study of the local electron density versus time for 1664 orbits revealed that in 132 orbits very sharp …

2009 Journal of Geophysical Research (Space Physics)
MEx VenusExpress 54
Midlatitude and high-latitude electron density profiles in the ionosphere of Saturn obtained by Cassini radio occultation observations
DOI: 10.1029/2008JA013900 Bibcode: 2009JGRA..114.4315K

Nagy, A. F.; Kliore, A. J.; Marouf, E. A. +4 more

Nineteen new radio occultations of the ionosphere of Saturn have been obtained since 2006. Sixteen of these occultations were from midlatitude and high latitudes and thus provided important, new information of the ionosphere for these regions. A high degree of variability in the electron densities were observed, but grouping and averaging the obse…

2009 Journal of Geophysical Research (Space Physics)
Cassini 48
Source locations of narrowband radio emissions detected at Saturn
DOI: 10.1029/2008JA013855 Bibcode: 2009JGRA..114.6219Y

Gurnett, D. A.; Hospodarsky, G. B.; Kurth, W. S. +7 more

Since Cassini's arrival at Saturn in 2004, the Radio and Plasma Wave Science instrument has detected numerous narrowband (NB) radio emission events. These emissions, mostly detected around 5 and 20 kHz, usually occur periodically for several days after intensifications of Saturn kilometric radiation. We present calculations based on an electron de…

2009 Journal of Geophysical Research (Space Physics)
Cassini 47
Spatial structures of magnetic depression in the Earth's high-altitude cusp: Cluster multipoint observations
DOI: 10.1029/2009JA014283 Bibcode: 2009JGRA..11410202S

Zhang, H.; Zong, Q. -G.; Lucek, E. +11 more

Magnetic depression structures (magnetic holes) of short time duration from seconds to minutes have been studied using Cluster data in the high-latitude cusp. Our multispacecraft analysis revealed that the magnetic depressions are spatial structures traveling across the spacecraft, and this result was further strengthened by the calculation of the…

2009 Journal of Geophysical Research (Space Physics)
Cluster 47