Magnetic Field in a Turbulent Galactic Disk
1990 ◽
Vol 140
◽
pp. 157-158
Keyword(s):
A numerical model of magnetic field structure in the presence of turbulent motions of the interstellar gas has been made. We solved the kinematic equation of magnetic field transport in a limited volume of ISM. Diffusion effects smoothing out small-scale structure are allowed as well. A permanent helical configuration of field lines has been found. This justifies, at least partly, searching solutions in the dynamo theory in the form of field modes. The presence of diffusion appears essential for the time evolution of magnetic field and magnetic energy density.
2012 ◽
Vol 08
◽
pp. 364-367
2010 ◽
Vol 6
(S273)
◽
pp. 233-241
◽
Keyword(s):
2010 ◽
Vol 6
(S274)
◽
pp. 445-448
2021 ◽
Vol 502
(2)
◽
pp. 2807-2814
1970 ◽
Vol 41
(2)
◽
pp. 435-452
◽
Keyword(s):
1993 ◽
Vol 141
◽
pp. 143-146
Keyword(s):
1993 ◽
Vol 157
◽
pp. 283-297
Keyword(s):
1976 ◽
Vol 71
◽
pp. 323-344
◽
Keyword(s):