From: The competition between Lorentz and Coriolis forces in planetary dynamos
Λ i | Λ d | \(\Lambda _{d}^{*}\) | Λ I | Λ P |
---|---|---|---|---|
\(\frac {B^{2}}{2 \rho _{o} \mu _{o} \eta \Omega }\) | \(\frac {\Lambda _{i}}{Rm} \frac {D}{\ell _{B}}\) | \( 0.77 \frac {\Lambda _{i}}{Rm^{1/2}}\) | \(\frac {\int _{V}{|\mathbf {F_{L}}| dV}}{\int _{V}{|\mathbf {F_{C}}| dV}}\) | \(\frac {|\mathbf {F_{L}}|}{|\mathbf {F_{C}}|}\), max probability |