Diffusive spreading of dynamo fields into turbulent exteriors reverses the usual decay ordering, allowing quadrupole toroidal components to decay slower than dipoles and confining fields within a magnetosphere whose synchrotron signatures are potentially observable.
year = 1957, month = sep, volume =
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The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.
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Magnetic field spreading from stellar and galactic dynamos into the exterior
Diffusive spreading of dynamo fields into turbulent exteriors reverses the usual decay ordering, allowing quadrupole toroidal components to decay slower than dipoles and confining fields within a magnetosphere whose synchrotron signatures are potentially observable.
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The Accretion Process on Protostars
The paper reviews techniques for measuring protostellar accretion, analyzes methodological differences and caveats in comparing observations with simulations, and outlines next steps for a fuller picture.