Computer Science
Scientific paper
Mar 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975icar...24..311s&link_type=abstract
Icarus, vol. 24, Mar. 1975, p. 311-324.
Computer Science
10
Planetary Atmospheres, Planetary Environments, Planetary Magnetic Fields, Planetary Magnetospheres, Uranus (Planet), Atmospheric Models, Dipole Moments, Interplanetary Medium, Magnetic Moments, Outer Planets Explorers, Solar Wind Velocity
Scientific paper
In 1985 the spin axis of Uranus points within 10 degrees of the sun and the planet's position is very near the solar apex direction. A Uranus mission with an encounter near 1985 might expect to measure the unusual particle and field configuration of a 'pole-on' magnetosphere and also properties of the interstellar medium. Estimates are given of the particle and field environment of Uranus based on extrapolation of solar-wind data from 1 AU and on scaling relations for an earth-type magnetosphere. Since the magnetic moment of Uranus is unknown, all magnetospheric parameters are derived as a function of the dipole strength. The onsets of special magnetospheric properties are identified as the dipole moment increases from small to large values. A fairly complete set of magnetospheric parameters is given for a specific dipole moment to illustrate the case of a large moment.
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