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Turbulence, magnetic fields, and plasma physics in clusters of galaxiesa)
a)Paper RI1b 2, Bull. Am. Phys. Soc. 50, 306 (2005).
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10.1063/1.2179053
/content/aip/journal/pop/13/5/10.1063/1.2179053
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/5/10.1063/1.2179053

Figures

Image of FIG. 1.
FIG. 1.

: solution of Eq. (11) calculated numerically for the cool-core parameters of Table I.

Image of FIG. 2.
FIG. 2.

The mechanism of the fluctuation dynamo.

Image of FIG. 3.
FIG. 3.

Evolution of the magnetic-field strength for the cool-core parameters of Table I.

Image of FIG. 4.
FIG. 4.

Cross sections of (left) and (right) in the saturated state of a simulation with , (run B of Ref. 69).

Image of FIG. 5.
FIG. 5.

A schematic illustration of the structure of cluster turbulence proposed in Sec. VI.

Tables

Generic image for table
Table I.

Cluster parameters.

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/content/aip/journal/pop/13/5/10.1063/1.2179053
2006-05-08
2014-04-19
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752b84549af89a08dbdd7fdb8b9568b5 journal.articlezxybnytfddd
Scitation: Turbulence, magnetic fields, and plasma physics in clusters of galaxiesa)
http://aip.metastore.ingenta.com/content/aip/journal/pop/13/5/10.1063/1.2179053
10.1063/1.2179053
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