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Table 1.

Summary of key parameters, governing integration terms, and predictive skills of selected solar dynamo models.

Model 1 Model 2 Model 3 Model 4 Model 5
Parameters:
Ω Eq. (4) of DC99 Eqs. (20-21) of PC20 Eqs. (20-21) of PC20 Eq. (10-11) of ZJ22 Eq. (10-11) of ZJ22
Up Eq. (5) of DC99 Eq. (5) of DC99 / Eq. (12) of ZJ22 /
η Eq. (6) of DC99 Eq. (22) of PC20 Eq. (22) of PC20 Eq. (14) of ZJ22 Eq. (14) of ZJ22
S Eq. (7) of DC99 Eq. (5-8) of CB11 Eq. (5-9) of CB11 Eq. (6-9) of ZJ22 Eq. (6-9) of ZJ22
γ / / / Eq. (13) of ZJ22 Eq. (13) of ZJ22
Integration term dominating d Φ N dt Mathematical equation: $ \frac{d\Phi^N}{dt} $ I1 I1 I2 + I3 I1 I1
Exhibits predictive skill Yes Yes No Yes Yes
Physical mechanism for the predictive skill The surface poloidal field is efficiently coupled back into the dynamo loop The surface poloidal field is efficiently coupled back into the dynamo loop / The surface magnetic field represents the radial component of the interior poloidal field The surface magnetic field represents the radial component of the interior poloidal field

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