Low-frequency Jovian emission and solar wind magnetic sector structure

Details Low-frequency Jovian emission and solar wind magnetic sector structure Low-frequency Jovian emission and solar wind magnetic sector structure

Jan 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984natur.306..767z&link_type=abstract

Nature (ISSN 0028-0836), vol. 306, Jan. 4, 1984, p. 767, 768.

Astronomy and Astrophysics

Astronomy

27

Extraterrestrial Radio Waves, Interplanetary Magnetic Fields, Jupiter Atmosphere, Planetary Radiation, Solar Planetary Interactions, Solar Wind, Kilometric Waves, Periodic Variations, Planetary Magnetospheres, Voyager Project

Scientific paper

Observations from the Planetary Radio Astronomy experiment aboard the two Voyager spacecraft are used to study the long-term fluctuations of the Jovian emission at hectometer and kilometer wavelengths. A power spectrum analysis of the data leads to the conclusion that the sector structure of the interplanetary magnetic field has an important role in controlling the long-term intensity fluctuations observed at hectometer wavelengths and the correlated variations of the broad-band emissions at kilometer wavelengths. The position of the sources of emission in the Jovian magnetosphere is discussed.

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