Non-Axisymmetric Magnetic Structure Generation in Planets Sun and Galaxies
1993 ◽
Vol 157
◽
pp. 263-267
Keyword(s):
The problem of preferential excitation of non-axially symmetric magnetic fields in most of the observed spiral galaxies and in planets as Uranus and Neptune is studied. It is suggested that a dynamo acting in a thin conductive shell is possible in these objects.It is shown that in this thin shell axisymmetric and non-axisymmetric magnetic field modes can be excited with equal efficiency. The preferential excitation of non-axially symmetric magnetic fields is possible, when the gradient of the angular velocity of rotation is comparatively small and has an essential component perpendicular to the shell.
1969 ◽
Vol 1
(6)
◽
pp. 274-276
◽
1990 ◽
Vol 140
◽
pp. 177-181
◽
Keyword(s):
1974 ◽
Vol 64
◽
pp. 187-187
1990 ◽
Vol 140
◽
pp. 83-89
1990 ◽
Vol 140
◽
pp. 233-234
Keyword(s):
1990 ◽
Vol 140
◽
pp. 241-241
2020 ◽
Vol 117
(11)
◽
pp. 5638-5643
◽
Keyword(s):
2018 ◽
Vol 44
(19)
◽
pp. 66
Keyword(s):
2010 ◽
Vol 6
(S274)
◽
pp. 389-392
2010 ◽
Vol 6
(S274)
◽
pp. 381-384
Keyword(s):