The first three-dimensional reconstruction of a celestial object at radio wavelengths: Jupiter's radiation belts.

Details The first three-dimensional reconstruction of a celestial object at radio wavelengths: Jupiter's radiation belts. The first three-dimensional reconstruction of a celestial object at radio wavelengths: Jupiter's radiation belts.

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...324.1190s&link_type=abstract

Astronomy and Astrophysics, v.324, p.1190-1196

Astronomy and Astrophysics

Astrophysics

19

Planets And Satellites: Individual: Jupiter, Techniques: Interferometric, Methods: Data Analysis

Scientific paper

For an object where the emission is optically thin, it is shown that the visibility measured by an interferometer is a sample of the three-dimensional Fourier transform of the object. If the object rotates, then it is possible to sample this three-dimensional Fourier space adequately, and so reconstruct the object in three dimensions. Using this principle, reconstructions of Jupiter's synchrotron radiation belts can be formed. This paper considers the principle and practice of this reconstruction process.

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