Dynamo quenching is the reduction or modification of magnetic-field generation by magnetic feedback on the generating flow and its correlations. The Lorentz force can change shear or turbulence, while magnetic helicity affects mean-field regeneration. A phenomenological scalar example is . In the illustrative amplitude equation with , a growing field saturates at when . This demonstrates the negative feedback mechanism without claiming that algebraic quenching is a complete solar closure.
Algebraic alpha quenching prescribes a field-dependent alpha effect as a closure for nonlinear mean-field dynamo feedback. The polynomial law with decreases alpha, so it can saturate positive alpha but makes negative alpha more negative. It therefore differs importantly from the sign-preserving rational law . Its solutions must satisfy nonnegative squared-amplitude conditions; an assertion based only on large need not hold for both signs.
A rotating wave in a complex dynamo quenching model has constant amplitude and a common phase factor . In the two-hemisphere model with toroidal coupling parameter , eliminating the poloidal amplitudes gives
The matrix is Hermitian, so its eigenvalue is real and a nonzero rotating wave with has . Writing , pure dipole and quadrupole waves have and , respectively, when those quantities are positive.
For nonzero coupling , an alpha-quenching rotating wave can be made real in its toroidal amplitudes by a common phase rotation. Set . The amplitude equations are and . Subtracting after cross multiplication gives . Unequal magnitudes therefore require and . They exist exactly when and have the displayed squared amplitudes. Exchanging hemispheres yields the companion solution. This breaks equatorial reflection symmetry and combines both dipole and quadrupole parity in a mean-field dynamo. Existence does not alone prove nonlinear stability.

Articles by others on the same topic (0)

There are currently no matching articles.