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AGU: Geophysical Research Letters

 

Index Terms

  • Planetary Sciences: Solar System Objects: Saturn
  • Planetary Sciences: Solar System Objects: Saturnian satellites
  • Space Plasma Physics: Transport processes

Abstract

GEOPHYSICAL RESEARCH LETTERS, VOL. 32, L14S03, 4 PP., 2005
doi:10.1029/2005GL022654

Discovery of nitrogen in Saturn's inner magnetosphere

H. T. Smith

Engineering Physics, University of Virginia, Charlottesville, Virginia, USA

M. Shappirio

Goddard Space Flight Center, Greenbelt, Maryland, USA

E. C. Sittler

Goddard Space Flight Center, Greenbelt, Maryland, USA

D. Reisenfeld

Department of Physics and Astronomy, University of Montana, Missoula, Montana, USA

R. E. Johnson

Engineering Physics, University of Virginia, Charlottesville, Virginia, USA

R. A. Baragiola

Engineering Physics, University of Virginia, Charlottesville, Virginia, USA

F. J. Crary

Southwest Research Institute, San Antonio, Texas, USA

D. J. McComas

Southwest Research Institute, San Antonio, Texas, USA

D. T. Young

Southwest Research Institute, San Antonio, Texas, USA

We detected N+ in Saturn's magnetosphere in the range L ∼ 3.5 to ∼9.5 Saturn Radii (Rs) using data collected by the Cassini Plasma Spectrometer during Saturn Orbit Insertion and the following orbit (Rev A). The presence of N+ in Saturn's magnetosphere has been a source of much debate since Voyager's detection of unresolved mass/charge 14–16 amu ions in this region. Two principal nitrogen sources have been suggested: Titan's atmosphere and nitrogen compounds trapped in Saturn's icy satellite surfaces ( Sittler et al., 2004; E. C. Sittler et al., Energetic nitrogen ions within the inner magnetosphere of Saturn, submitted to Journal of Geophysical Research, 2004 ). The latter may contain primordial nitrogen, likely as NH3 in ice (Stevenson, 1982; Squyers et al., 1983) or N+ that has been implanted in the surface (Delitsky and Lane, 2002). In addition to our nitrogen detection results, we also present an initial examination of possible sources of these ions.

Received 7 February 2005; accepted 22 March 2005; published 3 June 2005.

Citation: Smith, H. T., M. Shappirio, E. C. Sittler, D. Reisenfeld, R. E. Johnson, R. A. Baragiola, F. J. Crary, D. J. McComas, and D. T. Young (2005), Discovery of nitrogen in Saturn's inner magnetosphere, Geophys. Res. Lett., 32, L14S03, doi:10.1029/2005GL022654.

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