The differential rotation rate of the Sun is usually described by the equation ω = A – B sin^2(φ) – C sin^4(φ), where ω is the angular velocity, φ is the latitude, and A, B, and C are constants.
Data, Tables, Tools, Guides
The differential rotation rate of the Sun is usually described by the equation ω = A – B sin^2(φ) – C sin^4(φ), where ω is the angular velocity, φ is the latitude, and A, B, and C are constants.