and also recently confirmed, the Galactic center region contains highly regular magnetic fields with strengths up to 1 mG. This extremely intensive field is concentrated in thin filaments oriented perpendicularly to the Galactic plane. The characteristic length of these filaments is about 0.5 kpc.]{}

-   [The local Galactic field is oriented mainly parallel to the plane, with a vertical component of only $B_z \simeq (0.2 \div 0.3)$ $\mu$G in vicinity of the Sun. The recent explanation is that this component is present due to existence of poloidal magnetic field (see theoretical global field model below) — poloidal field naturally originates within dynamo model of GMF generation.]{}

-   [The Galaxy is surrounded by a thick radio disk (height of about 1.5 kpc above and under Galactic plane, half-width of 300 pc) similar to that of the edge-on spiral galaxies. The field strength in this thick disk is estimated to be around 1 $\mu$G. As in the case of vertical field component discussed above (poloidal field), the most common explanation of existence of such thick disc is that this field is toroidal field originating through dynamo effect.]{}

-   [The local Galactic field in the standard thin disk has an even symmetry with 