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Jupiter, as observed at short radio wavelengths
1965
Journal of Research of the National Bureau of Standards Section D Radio Science
The history of our knowledge of the microwave emission from Jupiter is reviewed brie fly , hi gh· lighting only what appear to the reviewer to be the significant advances. The Van Allen belt emisSion has a constant flux density, and polarization from 200 Mc/s to 3000 Mc/s, but probably d ecrea ses at frequencies above 3000 Mc/s. The radiation from the di s k co rre s ponds to near inf~ared temperatures at wavelengths of a few centimeters, but may increase at longe r wave le ngths, reachll1g tWi
doi:10.6028/jres.069d.165
fatcat:pvv7ao5jubb2bjj7s67c6cbu5q