Saturn emits bursts of radio waves from its polar regions as it rotates. This study examines how the solar wind affects the intensity and periodicity of the radio bursts. The results not only show how Saturn's magnetosphere interacts with the solar wind, but they also provide a framework for understanding radio emissions from extrasolar planets and pulsars
Saturn has often been described as intermediate between Earth and Jupiter in terms of its magnetosph...
Saturn narrowband (NB) radio emissions are detected between 3 and 70 kHz, with occurrence probabilit...
During the period 8 to 30 January 2004, a campaign to study the correlation between the solar wind a...
International audienceThe internal rotation rates of the giant planets can be estimated by cloud mot...
Saturn is a source of intense kilometre-wavelength radio emissions that are believed to be associate...
Voyager spacecraft radio, interplanetary plasma, and interplanetary magnetic field data are used to ...
With the arrival of the Cassini spacecraft at Saturn in July 2004, there have been quasi-continuous ...
The discovery of Saturn kilometric radiation (SKR) was made by the Voyager spacecraft over three dec...
International audienceThe Unified Radio and Plasma Wave (URAP) experiment on the interplanetary spac...
International audienceWe propose an explanation for the variations at the 1% level of Saturn's radio...
Intense saturnian radio emission has been observed since June 2004, and until today, by the Radio an...
International audienceIntense saturnian radio emission has been observed since June 2004, and until ...
International audienceWith the arrival of the Cassini spacecraft at Saturn in July 2004, there have ...
International audienceSimilar to past studies at Jupiter, we conduct an investigation of possible as...
We report on radio signatures observed at Saturn by the Cassini RPWS experiment which are strikingly...
Saturn has often been described as intermediate between Earth and Jupiter in terms of its magnetosph...
Saturn narrowband (NB) radio emissions are detected between 3 and 70 kHz, with occurrence probabilit...
During the period 8 to 30 January 2004, a campaign to study the correlation between the solar wind a...
International audienceThe internal rotation rates of the giant planets can be estimated by cloud mot...
Saturn is a source of intense kilometre-wavelength radio emissions that are believed to be associate...
Voyager spacecraft radio, interplanetary plasma, and interplanetary magnetic field data are used to ...
With the arrival of the Cassini spacecraft at Saturn in July 2004, there have been quasi-continuous ...
The discovery of Saturn kilometric radiation (SKR) was made by the Voyager spacecraft over three dec...
International audienceThe Unified Radio and Plasma Wave (URAP) experiment on the interplanetary spac...
International audienceWe propose an explanation for the variations at the 1% level of Saturn's radio...
Intense saturnian radio emission has been observed since June 2004, and until today, by the Radio an...
International audienceIntense saturnian radio emission has been observed since June 2004, and until ...
International audienceWith the arrival of the Cassini spacecraft at Saturn in July 2004, there have ...
International audienceSimilar to past studies at Jupiter, we conduct an investigation of possible as...
We report on radio signatures observed at Saturn by the Cassini RPWS experiment which are strikingly...
Saturn has often been described as intermediate between Earth and Jupiter in terms of its magnetosph...
Saturn narrowband (NB) radio emissions are detected between 3 and 70 kHz, with occurrence probabilit...
During the period 8 to 30 January 2004, a campaign to study the correlation between the solar wind a...