Dynamo and Fossil Magnetic Field in Young Stars
1993 ◽
Vol 157
◽
pp. 171-175
Keyword(s):
The theory of fossil magnetic fields shows that new born stars may have internal magnetic fields of more than 1 million gauss. Convection inside young solar type stars will tangle any strong fossil magnetic field. The small scale magnetic field rises to the surface and determines the young stars activity attenuating with their age. When a fossil field is diminished a turbulent dynamo may begin to work in the condition of nonlinear stabilization. The scaling relations for the turbulent αω dynamo show that the strength of the generated “fossil” magnetic field inside the main sequence stars is stabilized on the level one tenth — 10 millions gauss, depending on the mass of the stars.
1994 ◽
Vol 162
◽
pp. 184-185
1988 ◽
Vol 132
◽
pp. 309-312
Keyword(s):
1991 ◽
Vol 130
◽
pp. 151-153
1981 ◽
Vol 93
◽
pp. 257-272
◽
Keyword(s):
1983 ◽
Vol 102
◽
pp. 417-438
Keyword(s):
2007 ◽
Vol 328
(6)
◽
pp. 475-490
◽