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Sökning: id:"swepub:oai:DiVA.org:uu-218772" > On the structure an...

On the structure and dynamics of Saturn's inner plasma disk

Holmberg, Mika (författare)
Uppsala universitet,Institutionen för fysik och astronomi,Astronomy and Space Physics
Wahlund, Jan-Erik, Associate professor (preses)
Uppsala universitet,Institutet för rymdfysik, Uppsalaavdelningen
Lebreton, Jean-Pierre, Professor (opponent)
CNRS-Orléans
 (creator_code:org_t)
Uppsala : Uppsala universitet, 2013
Engelska 57 s.
  • Licentiatavhandling (övrigt vetenskapligt/konstnärligt)
Abstract Ämnesord
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  • This licentiate thesis presents our investigation of Saturn's inner plasma disk. The thesis gives an overview of the Cassini-Huygens project, what a plasma is and how we use the Langmuir probe to investigate it, various difficulties related to the measurements, the structure of the magnetosphere of Saturn, with special focus on the inner magnetosphere and the region around the Saturnian moon Enceladus. For our investigation we use the Cassini Langmuir probe to derive ion density and ion velocity in the region from 2.5 to 12 Saturn radii. We show that the dominant part of the plasma torus, ion density above ~15 particle/cm3, is located in between 2.5 and 8 Saturn radii (1 RS = 60,268 km) from the planet, with a north-southward extension of 2 RS. The plume of the moon Enceladus is clearly visible as an ion density maximum of 105 cm-3, only present at the south side of the ring plane, as expected since the Enceladus plumes are located in the south polar region. Also the azimuthal ion velocity vi,Θ is estimated, showing a clear general trend in the region between 3 and 7 RS, described by vi,Θ =1.5R2-8.7R+39. The average vi,Θ starts to deviate from corotation speed at around 3 RS and reaches down to ~68 % of corotation close to 5 RS. The Langmuir probe data show a clear day/night side asymmetry in both ion density and ion velocity, most prominent in the radial region 4-6 RS from the center of Saturn. The ion densities ni varies from an average of ~35 cm-3 for the lowest dayside values close to noon up to ~70 cm-3 for the highest nightside values around midnight. The azimuthal ion velocities vi,Θ varies from ~28-32 km/s at the lowest dayside values around noon to ~36-40 km/s at the highest nightside values around midnight. This gives an azimuthal ion velocity difference between noon and midnight of Δvi,Θ ~5-10 km/s. The day/night asymmetry is suggested to be due to dust-plasma interaction.

Nyckelord

Saturn
E-ring
plasma disk
Space and Plasma Physics
Rymd- och plasmafysik

Publikations- och innehållstyp

vet (ämneskategori)
lic (ämneskategori)

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