On the radio emission of Callisto |
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| Authors: | AD Kuzmin BYA Losovsky |
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| Institution: | Lebedev Physical Institute, USSR Academy of Sciences, Moscow, USSR |
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| Abstract: | A model of an icy surface and interior for Callisto gives a predicted thermal radio emission in good agreement with experimental radio astronomical data. The radio brightness temperature of an icy surface will not depend on wavelength. This may be a method to test icy surface hypotheses. The brightness temperatures of other satellites with icy surfaces will be equal to 200–220°K and will not depend on wavelength. |
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