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The galactic dynamo and superbubbles

Part of: Macroscopic Randomness Focus on Plasma Astrophysics

Published online by Cambridge University Press:  17 December 2015

Russell M. Kulsrud
Russell M. Kulsrud*
Affiliation:
Princeton University, Department of Astrophysical Sciences, Princeton, NJ 08544, USA
*
†Email address for correspondence: rkulsrud@astro.princeton.edu
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Abstract

In previous galactic dynamo theories of the origin of the magnetic field in our galaxy, the subject of flux-freezing has been omitted. As a consequence, the equation of mass flow has generally also been omitted, particularly in the halo where the galactic gravitational field will operate on the mass flow. In this paper, it has been shown that this neglect could have serious consequences for the results obtained from those galactic dynamo simulations that include the halo. A modification of these dynamo theories is proposed which involves the expulsion of very small pieces of the magnetic field lines, rather than the wholesale expulsion of the complete magnetic lines encapsulated in the previous theories. This expulsion is accomplished by a spike instability that arises from superbubbles when they break out of the galactic disc and their shells fragment. This leads to a cut in the lines of force that still remain in the disc. Subsequently, normal disc turbulence rotates the cut lines and thus dissipates their mean flux, removing them from a role in the dynamo theory. This new process takes a length of time comparable to, but slightly longer than, the previous growth time of the disc dynamo, but avoids the previous difficulties associated with flux freezing and flux expulsion.

Type
Research Article
Information
Journal of Plasma Physics , Volume 81 , Issue 6 , December 2015 , 395810603
Copyright
© Cambridge University Press 2015 

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