Images of Jupiter's sulfur ring

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Photography, Jupiter (Planet), Rings, Sulfur, Io, Morphology, Plasma Dynamics, Time Response, Jupiter, Rings, Sulfur, Imagery, Characteristics, Satellites, Io, Shape, Plasmas, Temperatures, Magnetosphere, Emissions, Earth-Based Observations, Optical Properties, Sodium, Oxygen, Potassium, Photographs, Procedure, Radius, Magnetic Fields, Ions, Distance, Thickness, Ultraviolet Spectrometer, Voyager 1

Scientific paper

Images of the ring of singly ionized sulfur encircling Jupiter, obtained on two successive nights in April 1979, show that the ring characteristics may change dramatically in about 24 hr. On the first night the ring was narrow and confined to the magnetic equator inside Io's orbit. On the second night it was confined symmetrically about the centrifugal symmetry surface and showed considerable radial structure, including a 'fan' extending to Io's orbit. Many of the differences in the ring on the two nights can be explained in terms of differences in sulfur plasma temperature.

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