MAGNETOSPHERE

Although it is only about one-third the size of Jupiter’s magnetosphere,

Saturn’s magnetosphere is still an enormous structure, extending nearly

two million kilometers from the planet toward the Sun. The size of the

magnetosphere fluctuates rhythmically as the flow of charged particles

in the solar wind increases or decreases in intensity. The magnetosphere

can be pushed inside Titan’s orbit, so that at times the satellite finds

itself outside of the magnetosphere altogether.

Charged particles in the planet’s magnetosphere are dragged along by the

magnetic field, circling the planet at Saturn’s rotation rate of 10

hours, 39 minutes. These charged particles whiz by Titan at a dizzying

rate of more than 200 kilometers (120 miles) per second. Titan leaves a

motorboat-like wake in its orbital path.

Extending from the orbit of Titan inward to the orbit of Rhea, an

enormous cloud of uncharged hydrogen atoms forms a doughnut-shaped torus

of ultraviolet-emitting particles. Because of their neutrality, these

atoms are not towed around by Saturn’s magnetic field.

Close to the planet, Saturn’s rings act as an effective shield or

absorber of charged particles. The rings themselves are apparently

substantially affected in this process, however, as evidenced by their

“spokes” of fine particles and the lightning-like electrical discharges

attributed to the rings.

Voyager 1 Encounters Saturn · 第 20 / 25 题