Investigation Typical Jovian encounter objectives

Imaging science High-resolution reconnaissance over large

phase angles; atmospheric dynamics;

geologic structure of satellites

Infrared radiation Atmospheric composition, thermal

structure and dynamics; satellite surface

composition and thermal properties

Photopolarimetry Atmospheric aerosols; satellite surface

texture and sodium cloud

Radio science Atmospheric and ionospheric structure,

constituents, and dynamics

Ultraviolet spectroscopy Upper atmospheric composition and

structure; auroral processes;

distribution of ions and neutral atoms in

the Jovian system

Magnetic fields Planetary magnetic field; magnetospheric

structure; Io flux tube currents

Plasma particles Magnetospheric ion and electron

distribution; solar wind interaction with

Jupiter; ions from satellites

Plasma waves Plasma electron densities; wave-particle

interactions; low-frequency wave emissions

Planetary radio astronomy Polarization and spectra of radio

frequency emissions; Io radio modulation

process; plasma densities

Low-energy charged particles Distribution, composition, and flow of

energetic ions and electrons;

satellite-energetic particle interactions

Cosmic ray particles Distribution, composition, and flow of

high-energy trapped nuclei; energetic

electron spectra

[Illustration: A computer-generated mosaic of Voyager 1 pictures

showing Jupiter from directly above the north pole. This view shows

features to about 20 degrees south latitude. The black area at the

pole results from missing information.]

[Illustration: NASA]

Voyager Encounters Jupiter · 第 16 / 19 题