Very Large Array observations of Uranus at 2.0 CM

Details Very Large Array observations of Uranus at 2.0 CM Very Large Array observations of Uranus at 2.0 CM

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988aj.....96..388b&link_type=abstract

Astronomical Journal (ISSN 0004-6256), vol. 96, July 1988, p. 388-395.

Astronomy and Astrophysics

Astronomy

7

Image Processing, Uranus (Planet), Very Large Array (Vla), Very Long Base Interferometry, Brightness Temperature, Error Analysis, Voyager 2 Spacecraft

Scientific paper

Radio observations of Uranus obtained at 2.0 cm with the B configuration of the VLA during April 1985 are reported. The calibration and data-reduction procedures are described in detail, and the results are presented in tables, maps, and graphs and compared with IRIS 44-micron observations (Hanel et al., 1986). Features discussed include highest brightness centered on the pole rather than on the subearth point, a decrease in brightness temperature (by up to 9 K) at latitudes between -20 and -50 deg (well correlated with the IRIS data), and disk-center position (corrected for the observed radio asymmetry) in good agreement with that found on the basis of the outer contours of the image.

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