Mathematics – Logic
Scientific paper
Dec 1995
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995basi...23..481s&link_type=abstract
Bulletin of the Astronomical Society of India, Vol. 23, No. 4, p. 481 - 488
Mathematics
Logic
5
Magnetic Fields: Galaxies, Magnetic Fields: Origin, Galactic Dynamo, Turbulence, Magnetic Fields
Scientific paper
Magnetic fields correlated on several kiloparsec scales are seen in spiral galaxies. Their origin could be due to the winding up of a primordial cosmological field or due to amplification of a small seed field by a turbulent galactic dynamo. Both these options have difficulties. There is no known mechanism for producing the required primordial field. At the same time the turbulent dynamo may self-destruct before being able to produce the large scale field, due to excess of small scale power. The current status of these difficulties is discussed.
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