“…Higher resolution interferometric maps displayed with accuracy the regions of intense emission along the equator and at higher latitudes [ de Pater et al , 1982; de Pater and Jaffe , 1984; de Pater and Dickel , 1986; de Pater , 1981; Leblanc et al , 1997a], the brightness' dependence on the wavelength [ de Pater et al , 1982; de Pater and Dickel , 1986; de Pater , 1981; Leblanc et al , 1997a; de Pater and Dunn , 2003], longitude (east‐west asymmetry) [ de Pater , 1980; de Pater et al , 1982; de Pater and Jaffe , 1984; de Pater , 1981; Leblanc et al , 1997a], and D E (Earth's declination as seen from Jupiter) [ Dulk et al , 1999b]; and allowed a three‐dimenional reconstruction of Jupiter's synchrotron radiation [ Sault et al , 1997a; Leblanc et al , 1997a]. Observations at high resolution have proven to be valuable in constraining models for the magnetic field [ Dulk et al , 1997a, 1999a, 1999b] and the electron pitch angle and radial distributions [ de Pater , 1981; de Pater and Goertz , 1990; Levin et al , 2001; Garrett et al , 2005].…”