A new form of Saturn’s magnetopause using a dynamic pressure balance model, based on in situ, multi‐instrument Cassini measurement
Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through wh...
International audienceThe radio and plasma wave science (RPWS) experiment on board the Cassini space...
The Pioneer Saturn vector helium magnetometer has detected a bow shock and magnetopause at Saturn an...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95429/1/jgra19967.pd
The shape and location of a planetary magnetopause can be determined by balancing the solar wind dyn...
[1] The location and shape of a planetary magnetopause is principally determined by the dynamic pres...
We describe a new method of constructing an equilibrium magnetopause surface based on the pressure b...
International audienceSince the insertion of Cassini in the Saturnian system in July 2004, the radio...
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
International audienceTwo distinct and variable rotation periods in Saturn’s radio emissions were re...
In this thesis we show that Saturn’s magnetopause and bow shock oscillate with a period near that of...
Periodic variations have been observed in many field and particle properties in Saturn's magnetosphe...
This thesis describes how the structure and dynamics of Saturn’s magnetopause can be explored by mod...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through wh...
International audienceThe radio and plasma wave science (RPWS) experiment on board the Cassini space...
The Pioneer Saturn vector helium magnetometer has detected a bow shock and magnetopause at Saturn an...
Peer Reviewedhttp://deepblue.lib.umich.edu/bitstream/2027.42/95429/1/jgra19967.pd
The shape and location of a planetary magnetopause can be determined by balancing the solar wind dyn...
[1] The location and shape of a planetary magnetopause is principally determined by the dynamic pres...
We describe a new method of constructing an equilibrium magnetopause surface based on the pressure b...
International audienceSince the insertion of Cassini in the Saturnian system in July 2004, the radio...
The long-term statistical behavior of the large-scale structure of Saturn’s magnetosphere has been i...
We use magnetopause crossings of the Cassini spacecraft to study the response of Saturn's magnetosph...
International audienceTwo distinct and variable rotation periods in Saturn’s radio emissions were re...
In this thesis we show that Saturn’s magnetopause and bow shock oscillate with a period near that of...
Periodic variations have been observed in many field and particle properties in Saturn's magnetosphe...
This thesis describes how the structure and dynamics of Saturn’s magnetopause can be explored by mod...
We quantify the magnetospheric stress state of Saturn, revealing the nature of the planetary environ...
Magnetic reconnection is a fundamental process in solar system and astrophysical plasmas, through wh...
International audienceThe radio and plasma wave science (RPWS) experiment on board the Cassini space...
The Pioneer Saturn vector helium magnetometer has detected a bow shock and magnetopause at Saturn an...
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