Saturn's magnetic tail - Structure and dynamics

Details Saturn's magnetic tail - Structure and dynamics Saturn's magnetic tail - Structure and dynamics

Feb 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.292..753b&link_type=abstract

Nature, vol. 292, Aug. 20, 1981, p. 753-755.

Computer Science

28

Atmospheric Models, Geomagnetic Tail, Planetary Magnetic Fields, Planetary Magnetospheres, Plasma Interactions, Saturn Atmosphere, Solar Wind, Bow Waves, Shock Waves, Voyager 1 Spacecraft, Saturn, Structure, Dynamics, Magnetotail, Voyager 1, Magnetic Fields, Currents, Distribution, Comparisons, Observations, Models, Solar Wind, Magnetosphere, Data, Longitude, Interplanetary Magnetic Field, Velocity, Perturbations, Boundary Layers, Waves

Scientific paper

Voyager 1 magnetic field observations have provided evidence of a
Saturnian magnetic tail. Tail current system distributions are inferred
through comparison of the observations with a realistic magnetotail
current system model. Temporal variations observed in the tail were
probably produced by solar wind variations.

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