On August 18, 1999, Cassini flew by the Earth on its way to Saturn. The Cassini Earth swing-by was the fastest traversal of the Earth's magnetosphere to date. The spacecraft was traveling at 9.1 R-E hr(-1) (16.1 km s(-1)) and made rapid traversals of several regions of the terrestrial magnetosphere. During the Cassini Earth swing-by the Electron Spectrometer (ELS) collected almost 9 hours of data in the Earth's magnetosphere and almost 10 hours of solar wind data upstream of the Earth. During the pass, Cassini ELS sampled electrons in the solar wind, bow shock, magnetosheath, magnetopause, radiation belts, plasmasphere, plasma sheet, lobes, and crossings of the tail magnetopause. The purpose of this paper is (1) to give a summary of electro...
International audienceIn its Grand Finale phase, Cassini traversed a region of the Saturnian system ...
The Cassini F ring and Proximal orbits took the spacecraft closer to Saturn than any previous missio...
We study the energetic electrons by the Cluster-II Rapid instrument on a dayside high-latitude pass ...
The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-dimensional mass-resolved measu...
Unlike previous missions to the magnetotail (IMP 6, ISEE 1, ISEE 3, and Geotail), which effectively ...
We analyze electron plasma, energetic ion, and magnetic field data from four almost vertical Cassini...
International audienceAn electrostatic analyser (ESA) onboard the Equator-S spacecraft operating in ...
Pitch angle distributions (PADs) of very energetic electrons (110–365 keV) are examined during the r...
A new Cassini magnetosheath data set is introduced that is based on a comprehensive survey of interv...
International audienceIn its Grand Finale phase, Cassini traversed a region of the Saturnian system ...
The Cassini spacecraft orbited the planet Saturn from July 2004 to September 2017, and its varied or...
This thesis utilises data from the Cassini spacecraft in the analysis of the Saturnian system focusi...
We present an analysis of Saturn's inner plasmasphere as observed by the Cassini Plasma Spectrometer...
International audienceIn its Grand Finale phase, Cassini traversed a region of the Saturnian system ...
The Cassini F ring and Proximal orbits took the spacecraft closer to Saturn than any previous missio...
We study the energetic electrons by the Cluster-II Rapid instrument on a dayside high-latitude pass ...
The Cassini Plasma Spectrometer (CAPS) will make comprehensive three-dimensional mass-resolved measu...
Unlike previous missions to the magnetotail (IMP 6, ISEE 1, ISEE 3, and Geotail), which effectively ...
We analyze electron plasma, energetic ion, and magnetic field data from four almost vertical Cassini...
International audienceAn electrostatic analyser (ESA) onboard the Equator-S spacecraft operating in ...
Pitch angle distributions (PADs) of very energetic electrons (110–365 keV) are examined during the r...
A new Cassini magnetosheath data set is introduced that is based on a comprehensive survey of interv...
International audienceIn its Grand Finale phase, Cassini traversed a region of the Saturnian system ...
The Cassini spacecraft orbited the planet Saturn from July 2004 to September 2017, and its varied or...
This thesis utilises data from the Cassini spacecraft in the analysis of the Saturnian system focusi...
We present an analysis of Saturn's inner plasmasphere as observed by the Cassini Plasma Spectrometer...
International audienceIn its Grand Finale phase, Cassini traversed a region of the Saturnian system ...
The Cassini F ring and Proximal orbits took the spacecraft closer to Saturn than any previous missio...
We study the energetic electrons by the Cluster-II Rapid instrument on a dayside high-latitude pass ...