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- W1792157809 abstract "Abstract Measurements in Saturn's equatorial magnetosphere from mid‐2004 through 2013 made by Cassini's charge‐energy‐mass ion spectrometer indicate the presence of a rare, suprathermal (83–167 keV/e) ion species at Saturn with mass ~56 amu that is likely Fe + . The abundance of Fe + is only ~10 −4 relative to that of W + (O + , OH + , H 2 O + , and H 3 O + ), the water group ions which dominate Saturn's suprathermal and thermal ions along with H + and H 2 + . The radial variation of the Fe + partial number density (PND) is distinctly different from that of W + and most ions that comprise Saturn's suprathermal ion populations which, unlike thermal energy plasma ions, typically have a prominent PND peak at ~8–9 Rs (1 Saturn radius, Rs = 60,268 km). In contrast, the Fe + PND decreases more or less exponentially from ~4 to ~20 Rs , our study's inner and outer limits. Fe + may originate from metal layers produced by meteoric ablation near Saturn's mesosphere‐ionosphere boundary and/or possibly impacted interplanetary dust particles or the Saturn system's dark material in the main rings." @default.
- W1792157809 created "2016-06-24" @default.
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- W1792157809 date "2015-04-01" @default.
- W1792157809 modified "2023-10-14" @default.
- W1792157809 title "Discovery of suprathermal Fe <sup>+</sup> in Saturn's magnetosphere" @default.
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- W1792157809 doi "https://doi.org/10.1002/2014ja020906" @default.
- W1792157809 hasPublicationYear "2015" @default.
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