Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981natur.293..382g&link_type=abstract
Nature, vol. 293, Oct. 1981, p. 382, 383.
Astronomy and Astrophysics
Astronomy
8
Decametric Waves, Jupiter (Planet), Planetary Radiation, Radio Sources (Astronomy), Scintillation, Drift Rate, Interplanetary Magnetic Fields, Io, Lines Of Force, Jupiter, Scintillations, Source Medium, Emissions, Decameter Waves, Io, Wavelengths, Spectrum, Procedure, Techniques, Structure, Magnetic Fields, Drift Rate, Solar Wind, Origin
Scientific paper
A method based on the measurement of interplanetary scintillations which modulate Jovian decametric emissions received on the earth is proposed to study the structure and position of the emission source. The method involves the analysis of the frequency drift of interplanetary scintillation or the time delay between scintillation recorded at two different frequencies to obtain an apparent distance between sources. Preliminary results based on dynamic spectra obtained from wideband observations indicate that the emission is distributed in space and may occur along the magnetic field lines, and that the Io-controlled A and B sources are on opposite sides of Jupiter.
Boischot Andre
Genova Francoise
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