The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft has recorded abrupt increases in energetic neutral atom flux coming from the general direction of Saturn's magnetotail. These bursts of ion activity in the tail are well correlated with enhancements in the Saturn kilometric radiation. Given the similarities between these events and substorm activity on Earth, including their dependence on interplanetary conditions, we conclude that Earth-like substorms occur within Saturn's magnetosphere
Recently, rotationally driven magnetic reconnection was first discovered in Saturn's dayside magneto...
Planetary magnetospheres receive plasma and energy from the Sun or moons of planets and consequently...
In July 2004 the Cassini spacecraft began its orbital tour in the Saturnian system and performed 74 ...
The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft...
Energetic particles (>∼25 keV) have been observed routinely in the terrestrial magnetosheath, but ha...
We use particle and magnetic field data from the Ion and Neutral Camera (INCA) and the magnetometer ...
[1] We present Cassini Visual and Infrared Mapping Spectrometer observations of infrared auroral emi...
International audienceWith the arrival of the Cassini spacecraft at Saturn in July 2004, there have ...
We give an overview of the charged and neutral particle measurements during the Grand Finale of Cass...
Plasmoids in Saturn's magnetotail are identified by a reversal (northward turning) of the normally s...
One of the primary Cassini mission objectives at Saturn is to characterize Saturn's aurora-its spati...
We present a case study of an event from August 20th (day 232) of 2006, when the Cassini spacecraft ...
Considerable observational evidence is found that ions are accelerated to high energies in the outer...
Saturn's morningside auroras consist mainly of rotating, transient emission patches, following perio...
We present a case study of an event from 20 August (day 232) of 2006, when the Cassini spacecraft wa...
Recently, rotationally driven magnetic reconnection was first discovered in Saturn's dayside magneto...
Planetary magnetospheres receive plasma and energy from the Sun or moons of planets and consequently...
In July 2004 the Cassini spacecraft began its orbital tour in the Saturnian system and performed 74 ...
The Magnetospheric Imaging Instrument (MIMI) Ion and Neutral Camera (INCA) on the Cassini spacecraft...
Energetic particles (>∼25 keV) have been observed routinely in the terrestrial magnetosheath, but ha...
We use particle and magnetic field data from the Ion and Neutral Camera (INCA) and the magnetometer ...
[1] We present Cassini Visual and Infrared Mapping Spectrometer observations of infrared auroral emi...
International audienceWith the arrival of the Cassini spacecraft at Saturn in July 2004, there have ...
We give an overview of the charged and neutral particle measurements during the Grand Finale of Cass...
Plasmoids in Saturn's magnetotail are identified by a reversal (northward turning) of the normally s...
One of the primary Cassini mission objectives at Saturn is to characterize Saturn's aurora-its spati...
We present a case study of an event from August 20th (day 232) of 2006, when the Cassini spacecraft ...
Considerable observational evidence is found that ions are accelerated to high energies in the outer...
Saturn's morningside auroras consist mainly of rotating, transient emission patches, following perio...
We present a case study of an event from 20 August (day 232) of 2006, when the Cassini spacecraft wa...
Recently, rotationally driven magnetic reconnection was first discovered in Saturn's dayside magneto...
Planetary magnetospheres receive plasma and energy from the Sun or moons of planets and consequently...
In July 2004 the Cassini spacecraft began its orbital tour in the Saturnian system and performed 74 ...