The mean-field electromotive force is the vector correlation $\mathcal{E}=⟨\mathbf{u}\times \mathbf{b}⟩$. Its curl enters the mean resistive induction equation. It is a local vector with units of velocity times magnetic field, not the scalar circuit voltage called electromotive force. A space-time average of periodic modes is often used to measure its transport coefficients.

The alpha effect is the part of a mean-field electromotive force linear in the mean magnetic field itself, $\mathcal{E}=\mathbf{\alpha }\overline{\mathbf{B}}+\cdots$. The alpha tensor can be anisotropic; it need not be a scalar multiple of the identity. Its curl can couple transverse mean-field components and produce an alpha-squared dynamo.

A Parker dynamo wave is a traveling or oscillatory mode of a mean-field dynamo coupling poloidal and toroidal magnetic-field components through an alpha effect and shear. A reduced complex-amplitude model can represent fluctuating alpha by a time-dependent coupling. Its periodically switched growth must be calculated from the monodromy matrix of a periodic linear system, rather than by averaging noncommuting generators.

First-order smoothing neglects the fluctuating nonlinear velocity-magnetic-field product in the fluctuation resistive induction equation, but retains $⟨\mathbf{u}\times \mathbf{b}⟩$ in the mean-field electromotive force. For a constant test field it gives ${\partial }_t\mathbf{b}-\eta {\nabla }^2\mathbf{b}=({\mathbf{B}}_0\cdot \nabla )\mathbf{u}$. Its validity requires the omitted terms to be small compared with the retained forcing and diffusion terms.

Differential rotation or shear stretches a poloidal magnetic field into a toroidal magnetic field. This is the Omega effect. By itself it need not regenerate the poloidal component; the alpha effect provides one possible feedback mechanism in an alpha-Omega dynamo. Without feedback, shear amplification can be transient or algebraic rather than sustained exponential dynamo action.

An alpha-Omega mean-field dynamo couples toroidal-field generation by the Omega effect to poloidal-field regeneration by the alpha effect. A simple Fourier model is $\dot{A}={\alpha }_{0}f(t)B-\eta k^{2}A$, $\dot{B}=ik\Omega A-\eta k^{2}B$, where $A$ is a component of the vector potential for the poloidal field and $B$ is a toroidal-field amplitude. For bounded $|f|\le 1$, the bounded-modulation alpha-Omega growth estimate controls the maximum amplification.

The second-order mean no-slip boundary condition correction contains products of first-order deformation modes and velocity gradients. Distinct integer wavenumbers have zero averaged mixed products. Their separate mean longitudinal and transverse contributions therefore add, even though mixed products create nonzero oscillatory flow modes.

A Lusin set is an uncountable subset $A$ of the real numbers such that $A\cap M$ is countable for every meagre set $M$. Every meagre subset has a meagre $F_{\sigma }$ cover, so testing those covers suffices. The Lusin set construction under CH gives an example. A Lusin set has no uncountable meagre subset of itself.

The complement of a comeagre set is a meagre set, a countable union of nowhere dense sets. A dense G-delta set is comeagre. The Baire category theorem ensures that two comeagre subsets of a nonempty complete metric space cannot be disjoint.

An uncountable subset of the real numbers with countable intersection with every meagre set. This is the category counterpart of a Sierpiński set.

An extendible geodesic is a geodesic segment that can be continued beyond at least one endpoint within the same manifold after retaining an affine parameter. An artificial truncation at a regular event is extendible even when its continuation eventually reaches a singularity.

Two rectangular matrices are related by invertible left and right multiplication exactly when their ranks agree. The rank-$r$ orbit in ${\mathrm{Mat}}_{b\times a}(k)$ has dimension $r(a+b-r)$: choose its image in a Grassmannian, then a surjective map to that image. These are the representation orbits of the one-arrow quiver.

An invertible complex Jordan block $\lambda I+N$, with $N^s=0$, has logarithm $\ell I+{\sum }_{k=1}^{s-1}(-1{)}^{k+1}(N/\lambda {)}^k/k$, where $e^{\ell }=\lambda$. Applying this construction blockwise and conjugating back proves surjectivity of the matrix exponential on the complex general linear group. There is no globally single-valued continuous choice of logarithm.

The Mathieu characteristic values are the parameter values $a$ for which the Mathieu equation has the even periodic mode traditionally denoted ${\mathrm{ce}}_n$, or the odd periodic mode ${\mathrm{se}}_n$. They are eigenvalues of $-d^2/d{t}^2+2q\cos 2t$ with the corresponding periodic or antiperiodic boundary conditions. Their small-$q$ expansions can be derived by projecting onto a Fourier series and perturbing the resulting tridiagonal matrix.

An ordinary massless spin-one particle has transverse vector polarizations under $SO(D-2)$. A covariant polarization satisfies $p\cdot ϵ=0$ and is identified under $ϵ\mapsto ϵ+\lambda p$. The quotient has $D-2$ positive polarizations.

A massive spin-one particle transforms as a vector under its massive particle little group $SO(D-1)$. Its $D-1$ polarizations are orthogonal to its timelike four-momentum. Under transverse $SO(D-2)$ rotations they split into a vector and a scalar.

For fixed cloud shape, gravitational energy scales as $-C_{g}G{M}^2/L$ and magnetic energy as $C_B{\Phi }^2/({\mu }_{0}L)$. The magnetic-criticality threshold for negligible pressure is $M/\Phi >\sqrt{C_B/C_g}/\sqrt{{\mu }_{0}G}$. Ideal flux freezing keeps this ratio fixed during homologous collapse; geometry determines the numerical coefficient.

For $T=-[\cos \varphi {]}_{-\infty }^{+\infty }/2$, complete the static energy into squares $({\varphi }_x\mp m\sin \varphi {)}^2$ and ${\sin }^2\varphi {\alpha }_x^2$. The boundary term is $\pm rmT$. A $T=1$ saturating kink is $\varphi =2\arctan e^{m(x-x_0)}$, with constant $\alpha$ and mass $rm$. This is a model-specific Bogomolny bound.

For $\alpha =\omega t+{\alpha }_0$ and $|\omega |<m$, the kink is $\varphi =2\arctan e^{\kappa (x-x_0)}$ with $\kappa =\sqrt{m^2-{\omega }^2}$. Its rest energy and mechanical internal charge are $M=r{m}^2/\kappa$ and $Q_0=r\omega /\kappa$. Eliminating the frequency gives the displayed mass relation. The orientation rotates while the energy profile remains stationary.

Locally this density is a total derivative, so it changes neither the bulk field equations nor the energy. Its contribution to the angular canonical momentum is a spatial boundary derivative. With ${ϵ}^{01}=+1$, it produces the theta-angle shift of a sigma-model kink charge.