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The author developed a thermoelectrical model of Solar system planets? magnetic fields and calculated Saturn?s magnetic field with its help. Radially directed thermoelectrical currents of the electroconductive layers of the planet are the essence of that model. The movement of those currents are determined by the intensity if the magnetic field, which is caused by the planetary thermogradient, e.g. the difference of temperature between the planet center and its outer shells of the electroconductive layers. The cal...