Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980pazh....6..305l&link_type=abstract
(Pis'ma v Astronomicheskii Zhurnal, vol. 6, May 1980, p. 305-308.) Soviet Astronomy Letters, vol. 6, May-June 1980, p. 168-170.
Astronomy and Astrophysics
Astronomy
Io, Planetary Evolution, Radiation Belts, Satellite Surfaces, Jupiter (Planet), Radiation Effects, Vaporizing
Scientific paper
Persistent or even continual localized eruptions of gas on Io could be produced through vaporization of surface material heated by infalling particles from the Jovian radiation belts. This process calls for a concentrated local particle influx, which could arise if Io has an intrinsic magnetic field of 0.02-1 gauss at the surface or if corresponding anomalies in its electrical conductivity are present. Seven of the nine eruption centers discovered on Io lie along a contour which is almost a great circle; probably it represents either a global fracture associated with magnetic anomalies or a feature analogous to the auroral oval on the earth.
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