Energetic ion characteristics and neutral gas interactions in Jupiter's magnetosphere
By B. Mauk, D. Mitchell, R. Mcentire, C. Paranicas, E. Roelof, Donald J. Williams, S. Krimigis, A. Lagg. 2004
254 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Molecular Biology
View Paper: https://www.semanticscholar.org/paper/e75e2b4d418d2d23e044304ac703356892ab142d
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Citations in the corpus
- INVARIANT KAPPA DISTRIBUTION IN SPACE PLASMAS OUT OF EQUILIBRIUM (2011, background): “…et al. 2004; 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;…”
- JUpiter ICy moons Explorer (JUICE): An ESA mission to orbit Ganymede and to characterise the Jupiter system (2013, background): “, 2003) and imaged in energetic neutral atom emissions onboard the Cassini spacecraft during its Jupiter flyby (Mauk et al., 2004).”
- Magnetospheric ion sputtering and water ice grain size at Europa (2013, background): “The much more energetic population is described by Mauk et al. (2004) and Paranicas et al. (2009).”
- The Jupiter Energetic Particle Detector Instrument (JEDI) Investigation for the Juno Mission (2017, background): “The Energetic Particle Detector (EPD) on the Galileo mission to Jupiter (Williams et al. 1992) had a Microchannel Plate (MCP) sensor similar to that of JEDI, and it was shielded with metal shielding with a mass thickness of about 5 g/cm2.”
- Simultaneous Chandra X ray, Hubble Space Telescope Ultraviolet, and Ulysses Radio Observations of Jupiter's Aurora (2005, background): “Mauk et al., 2002, 2004 ], this in turn requires that the ions undergo significant field-aligned A01207 ELSNER ET AL.: CHANDRA’S OBSERVATION OF JUPITER’S AURORA”