Paper
7 October 1996 Cassini plasma spectrometer investigation
David T. Young, Bruce L. Barraclough, Jean-Jacques Berthelier, M. Blanc, J. L. Burch, A. J. Coates, Raymond M. Goldstein, Manuel Grande, Tom W. Hill, J. M. Illiano, M. A. Johnson, R. E. Johnson, R. A. Baragiola, V. Kelha, D. Linder, David J. McComas, Bjoern T. Narheim, Jane E. Nordholt, A. Preece, E. C. Sittler, K. R. Svenes, Sandor Szalai, K. Szego, P. Tanskanen, K. Viherkanto
Author Affiliations +
Abstract
Cassini/Huygens is a joint project of NASA and the European Space Agency designed to explore the Saturnian system in depth during its four-year mission. Cassini, the orbiter spacecraft, will carry twelve hardware investigations while Huygens, the Titan atmospheric probe, will carry an additional six. The Cassini Plasma Spectrometer (CAPS), one of 12 orbiter investigations, includes 3 plasma sensors designed to cover the broadest possible range of plasma energy, composition, and temporal variation. It is conservatively estimated that CAPS will provide a factor of ten or more improvement in measurement capabilities over those of the Voyager spacecraft at Saturn.
© (1996) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David T. Young, Bruce L. Barraclough, Jean-Jacques Berthelier, M. Blanc, J. L. Burch, A. J. Coates, Raymond M. Goldstein, Manuel Grande, Tom W. Hill, J. M. Illiano, M. A. Johnson, R. E. Johnson, R. A. Baragiola, V. Kelha, D. Linder, David J. McComas, Bjoern T. Narheim, Jane E. Nordholt, A. Preece, E. C. Sittler, K. R. Svenes, Sandor Szalai, K. Szego, P. Tanskanen, and K. Viherkanto "Cassini plasma spectrometer investigation", Proc. SPIE 2803, Cassini/Huygens: A Mission to the Saturnian Systems, (7 October 1996); https://doi.org/10.1117/12.253412
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Cited by 6 scholarly publications.
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KEYWORDS
Sensors

Ions

Plasma

Electrophoretic light scattering

Space operations

Electrons

Saturn

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