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Table: C-, P-, T-properties of the spin, the electromagnetic field, and their interactions.

	$\sigma$	B	E	curlB, $\dot{{\bf E}}$	$\mbox{\boldmath$\sigma$}\cdot{\bf B}$	$\mbox{\boldmath$\sigma$}\cdot{\bf E}$	$\mbox{\boldmath$\sigma$}\cdot{\rm curl}{\bf B}$ $\mbox{\boldmath$\sigma$}\cdot\dot{{\bf E}}$
C	$+$	$-$	$-$	$-$	$-$	$-$	$-$
P	$+$	$+$	$-$	$-$	$+$	$-$	$-$
T	$-$	$-$	$+$	$-$	$+$	$-$	$+$

Table: Vacuum, meduim and toroid contributions in (eV units) to neutrino oscillation at low energies, $E_\nu =10$ MeV

	$\Delta m^2/E_\nu$	$V_e$	$\tau\mbox{\boldmath$\sigma$}\cdot{\rm curl}\,{\bf B}$
Vacuum	$10^{-18}$	$-$	$10^{-31}\vert{\rm curl}{\bf B}\vert/1\,{\rm Gauss}\,{\rm cm}^{-1}$
Solar	$10^{-12}$	$10^{-11}$	$10^{-31}\vert{\rm curl}{\bf B}\vert/1\,{\rm Gauss}\,{\rm cm}^{-1}$

Figure Captions

Figure: Toroid form factors for $\nu _{e,\mu ,\tau }$ neutrinos vs the transverse momentum squared.
Figure: Born contributions to the $\nu + e \rightarrow \nu + e$ scattering.
Figure: Interference and toroid contributions to the $\nu _e e$ scattering cross-section.
Figure: Transition radiation at the interface of two media: $\nu (p_1) \rightarrow \nu (p_{2}) + \gamma (k)$. The refractive index changes from $n_{1}$ to $n_{2}$ at $z=0$.
Figure: Total energy in the medium-vacuum transition, $n_2=0$ and $n_i(\omega )\simeq 1-\omega _i^2/2\omega ^2$ for $\omega \gg \omega _i$ and $E_\nu =1$ MeV.