INVESTIGATION SATURN ENCOUNTER OBJECTIVES

Imaging science Planetary meteorology; satellite geology;

ring structure and dynamics

Infrared Atmospheric composition, thermal structure

interferometry and dynamics; satellite surface composition

and thermal properties; ring composition

Radio science Atmospheric and ionospheric structure,

constituents, and dynamics at Saturn and

Titan; ring particle size

Ultraviolet Upper atmospheric composition and structure;

spectroscopy auroral processes; distribution of ions and

neutral atoms in the Saturn system

Magnetic fields Planetary magnetic field; magnetospheric

structure

Plasma particles Magnetospheric ion and electron

distribution; solar wind interaction with

Saturn; ions from satellites

Plasma waves Plasma electron densities; wave-particle

interactions; low-frequency wave emissions

Planetary radio Polarization and spectra of radio-frequency

astronomy emissions; plasma densities

Low-energy charged Distribution, composition, and flow of

particles energetic ions and electrons;

satellite-energetic particle interactions

Cosmic ray particles Distribution, composition, and flow of

high-energy trapped nuclei; energetic

electron spectra

“_Notre voyageur connaissait merveilleusement les lois de la

gravitation, et toutes les forces attractives et répulsives. Il s’en

servait si à propos, que tantôt à l’aide d’un rayon de soleil, tantôt

par la commodité d’une comète, il allait de globe en globe, lui et les

siens, comme un oiseau voltige de branche en branche._”

“_Our voyager knew marvelously the laws of gravitation, and all

attractive and repulsive forces. He used them in such a timely way that,

once with the help of a ray of sunshine, another time thanks to a

cooperative comet, he went from globe to globe, he and his kin, as a

bird flutters from branch to branch._”

VOLTAIRE—Micromégas, Histoire Philosophique, 1752.

[Illustration: NASA]

Voyager 1 Encounters Saturn · 第 22 / 25 题