“…If, in addition, the field M (x, t) is solenoidal, i.e., (∇, M ) = 0, then the flux densities with numbers 1, 9, and 15 also vanish due to the divergence (∇, M ). As a result, under the unimodality and solenoidality conditions, the general equation Ṁj = L j [M ], which governs the dynamics of the field M and contains the differential operator described in Theorem 4.2 and the formula (4.1), takes the form Ṁj = f (2) − f (3) ΔM j + f (7) + f (8) ∇ k M j (M , ∇)M k + f (7) − f (8) ∇ k M k (M , ∇)M j + f (10) ∇ j M , [∇, M ] + f (11) + f (12) ∇ k [M , ∇] j M k + f (11) − f (12) ∇ k [M , ∇] k M j + ε jln f (13) + f (14) ∇ k (M n ∇ k M l ) + ε kln f (13) − f (14)…”