Ion densities and velocities in the inner plasma torus of Saturn
We present plasma data from the Cassini Radio and Plasma Wave Science (RPWS) Langmuir probe (LP), mapping the ion density and velocity of Saturn's inner plasma torus. Data from 129 orbits, recorded during the period from the 1st of February 2005 to the 27th of June 2010, are used to map the ext...
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Veröffentlicht in: | Planetary and space science 2012-12, Vol.73 (1), p.151-160 |
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Format: | Artikel |
Sprache: | eng |
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Zusammenfassung: | We present plasma data from the Cassini Radio and Plasma Wave Science (RPWS) Langmuir probe (LP), mapping the ion density and velocity of Saturn's inner plasma torus. Data from 129 orbits, recorded during the period from the 1st of February 2005 to the 27th of June 2010, are used to map the extension of the inner plasma torus. The dominant part of the plasma torus is shown to be located in between 2.5 and 8 Saturn radii (1RS=60,268km) from the planet, with a north-southward extension of ±2RS. The plasma disk ion density shows a broad maximum in between the orbits of Enceladus and Tethys. Ion density values vary between 20 and 125cm−3 at the location of the density maximum, indicating considerable dynamics of the plasma disk. The equatorial density structure, |z| |
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ISSN: | 0032-0633 1873-5088 1873-5088 |
DOI: | 10.1016/j.pss.2012.09.016 |