Stability against this process for a rotating star is given by the Ledoux Criterion, though if the density of stellar material is non-constant, the Solberg-Hoiland criterion is used instead since it adds a term dependent on the colatitude.
Stability against this process for a rotating star is given by the Ledoux Criterion, though if the density of stellar material is non-constant, the Solberg-Hoiland criterion is used instead since it adds a term dependent on the colatitude. The ";semi-"; form of this process occurs in regions with a molecular weight gradient, and can only occur if the differential of a certain quantity is less than gravity over heat capacity at constant pressure. This process only occurs if the Brunt- Vaisala frequency squared is less than zeroÂ—that frequency is often used to define the Schwarzschild criterion, which determines when this stellar process is stable. The tachocline is breached when this process's namesake ";overshoot"; moves parcels into the radiative zone. Turbulent ";granules"; on the Sun are produced by, for 10 points, what mechanism of energy transfer that predominates in the liquid component of stars?
Stability against this process for a rotating star is given by the Ledoux Criterion, though if the density of stellar material is non-constant, the Solberg-Hoiland criterion is used instead since it adds a term dependent on the colatitude.
stellar convection