Plasma Science From Fundamental Research to Technological Applications (1995) / Chapter Skim
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Pages 121-122
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From page 121... ...
Although the smallest relevant length scales are still unresolved by these calculations, the effects of buoyancy, concentration of flux into ropes, and dynamo activity all processes that are believed to play an important role in the dynamics of stellar magnetic fields are observed and can be studied. Formation of Low-Mass Stars It was recognized long ago that the ratio of magnetic flux to mass is much higher in the interstellar medium than it is in stars.
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From page 122... ...
v, 600 ~3 400 ~3 a' ._ D 200 Cot U) PLASMA SCIENCE Northwest ('~_ Faint sp 1 Plane of Sky A\ ~ 1 ~ o ·o -- l ~' .
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