Over 1989-2019, solar radio emission rotation periods increase from 22.49 days at 8800 MHz to 25.25 days at 245 MHz, indicating the corona rotates slower at higher altitudes.
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Study on the Temporal Evolution of the Radial Differential Rotation of Solar Corona Using Radio Emissions
Over 1989-2019, solar radio emission rotation periods increase from 22.49 days at 8800 MHz to 25.25 days at 245 MHz, indicating the corona rotates slower at higher altitudes.