Multi-instrument analysis of electron populations in Saturn's magnetosphere

By P. Schippers, M. Blanc, N. André, I. Dandouras, G. Lewis, L. Gilbert, A. Persoon, N. Krupp, Donald A. Gurnett, A. Coates and 3 more. 2008

361 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Molecular Biology

View Paper: https://www.semanticscholar.org/paper/67173f535f0981171924310e88ff808541dc69a5

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Citations in the corpus

Survey of ion plasma parameters in Saturn's magnetosphere (2010, background): “…the sum of the densities for the three species) with the published electron densities derived from CAPS/ELS data [Arridge et al., 2009, Figure 1; Schippers et al., 2008, Figure 3], from the upper hybrid line determination of RPWS [Schippers et al., 2008, Figure 3], and from the Languir probe on…”
INVARIANT KAPPA DISTRIBUTION IN SPACE PLASMAS OUT OF EQUILIBRIUM (2011, background): “…Leubner & Vörös 2005; Marsch 2006; Yoon et al. 2006; Pierrard & Lazar 2010) and the planetary magnetospheres (e.g., Christon 1987; Mauk et al. 2004; Schippers et al. 2008; Dialynas et al. 2009), in the outer heliosphere and the inner heliosheath (e.g., Decker & Krimigis 2003; Decker et al. 2005;…”
Kappa Distributions: Theory and Applications in Space Plasmas (2010, background): “…of Jupiter (Collier and Hamilton 1995), the magnetosphere of Jupiter (Krimigis et al. 1981; Mauk et al. 2004), Saturn (Krimigis et al. 1983; Schippers et al. 2008; Dialynas et al. 2009), Uranus (Krimigis et al. 1986), Neptune (Mauk et al. 1991), and even on Titan (De la Haye et al. 2007)…”
Introduction to special section on Origins and Properties of Kappa Distributions: Statistical Background and Properties of Kappa Distributions in Space Plasmas (2015, background): “…Christon, 1987; Wang et al., 2003; Kletzing et al., 2003], magnetospheric substorms [e.g., Hapgood et al., 2011], Saturnian magnetosphere [e.g., Schippers et al., 2008; Dialynas et al., 2009], and magnetospheres of planetary moons such as Io [e.g., Moncuquet et al., 2002] and Enceladus [e.g.,…”
Beyond kappa distributions: Exploiting Tsallis statistical mechanics in space plasmas (2009, background): “In fact, (39) was the first extracted distribution [Tsallis, 1988]. However, this result was highly problematic, mainly because it was not invariant for an arbitrary selection of the ground level of the energy. Subsequently, by considering the escort expectation values, Tsallis et al. [1998] succeed”