A copy of this work was available on the public web and has been preserved in the Wayback Machine. The capture dates from 2018; you can also visit the original URL.
The file type is application/pdf
.
The Centred Multipole and Other Representations of Jupiter's Magnetic Field
1976
Publications Astronomical Society of Australia
The fact that Jupiter's inner magnetosphere is not axially symmetric was originally demonstrated by ground-based radio measurements. Departures from symmetry are evident in the pattern of bursts occurring at decametre wavelengths and also in the characteristics of the polarized synchrotron emission observed at decimetre wavelengths. Direct measurements of Jupiter's magnetic field, made from the Pioneer space probes, also indicate departures from an axially symmetric configuration.
doi:10.1017/s1323358000014624
fatcat:zjnbu3f7izgbfnhkgz2jrisqwi