Jupiter's zone-belt structure at radio wavelengths. I - Observations

Details Jupiter's zone-belt structure at radio wavelengths. I - Observations Jupiter's zone-belt structure at radio wavelengths. I - Observations

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..459d&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 1, 1986, p. 459-466, 469-471. Research supported by the Alfred P

Astronomy and Astrophysics

Astrophysics

15

Jupiter (Planet), Planetary Radiation, Radio Emission, Thermal Emission, Planetary Environments, Planetary Magnetic Fields, Synchrotron Radiation

Scientific paper

VLA maps of Jupiter's thermal emission at 1.3, 2, 6, and 20 cm wavelengths are presented. The resolution at the four wavelengths is 0.218, 0.075, 0.108, and 0.144 Jovian radii respectively. Bright bands across the disk are clearly visible at 2 and 6 cm. These bands agree with the dark belts seen at optical and the bright bands seen at infrared wavelengths.

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