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ices Am 8; a line Aspects of two qualitative models of Enceladus ’ dust plume—the so-called ‘‘Cold Faithful’ ’ [Porco, C.C., et al., 2006. Cassini observes In 2004 the Cassini spacecraft entered its orbit around ring. Namely, the minimal vertical extent and the maximum particle number density of the...
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ftciteseerx:oai:CiteSeerX.psu:10.1.1.573.9859 2023-05-15T18:22:12+02:00 rg The Pennsylvania State University CiteSeerX Archives application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.573.9859 http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.573.9859 http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf text ftciteseerx 2016-01-08T12:40:06Z ices Am 8; a line Aspects of two qualitative models of Enceladus ’ dust plume—the so-called ‘‘Cold Faithful’ ’ [Porco, C.C., et al., 2006. Cassini observes In 2004 the Cassini spacecraft entered its orbit around ring. Namely, the minimal vertical extent and the maximum particle number density of the E ring were found near the orbit of Enceladus. Dynamical models for and Horányi, 2002). Moreover, the rather narrow size Porco et al., 2006; Spahn et al., 2006; Waite et al., 2006; Hansen et al., 2006). It turned out that Enceladus possesses an unusually ARTICLE IN PRESSwarm south pole which is characterized by a geologically young surface. The heat (at least as high as 140K, compared to expected 70K) is concentrated along the Text South pole Unknown South Pole |
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ices Am 8; a line Aspects of two qualitative models of Enceladus ’ dust plume—the so-called ‘‘Cold Faithful’ ’ [Porco, C.C., et al., 2006. Cassini observes In 2004 the Cassini spacecraft entered its orbit around ring. Namely, the minimal vertical extent and the maximum particle number density of the E ring were found near the orbit of Enceladus. Dynamical models for and Horányi, 2002). Moreover, the rather narrow size Porco et al., 2006; Spahn et al., 2006; Waite et al., 2006; Hansen et al., 2006). It turned out that Enceladus possesses an unusually ARTICLE IN PRESSwarm south pole which is characterized by a geologically young surface. The heat (at least as high as 140K, compared to expected 70K) is concentrated along the |
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The Pennsylvania State University CiteSeerX Archives |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.573.9859 http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf |
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http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf |
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http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.573.9859 http://www2.le.ac.uk/departments/mathematics/extranet/staff-material/staff-profiles/nb144/papers-1/BrilSchmSpa-PSS2008.pdf |
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Metadata may be used without restrictions as long as the oai identifier remains attached to it. |
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