Io-phase motion and jovian decametre source locations

Details Io-phase motion and jovian decametre source locations Io-phase motion and jovian decametre source locations

Mar 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978natur.272..339d&link_type=abstract

Nature, vol. 272, Mar. 23, 1978, p. 339, 340.

Astronomy and Astrophysics

Astronomy

1

Decametric Waves, Io, Planetary Radiation, Radio Astronomy, Jupiter (Planet), Noise Storms, Occultation, Phases

Scientific paper

A second-order effect in the relationship between jovian decameter storms and the departure of Io from superior geocentric conjunction is explained on the basis of latitudinal variations in the earth-Jupiter viewing geometry. These variations are defined by the 12-year cycle in the jovicentric declination of the earth. In addition, it is found that the emission of the jovian decameter storm source Io-B (Io-C) is beamed from the northern (southern) magnetic latitudes. These conclusions are compatible with source positions derived from polarimetry and from considerations of planetary-limb shadowing.

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