Collapsing star revs up magnetic fields
Channel: UC Berkeley
Date: 2015-11-30

Supercomputer visualization of the toroidal magnetic field in a collapsed, massive star, showing how in a span of 10 milliseconds the rapid differential rotation revs up the stars magnetic field to a million billion times that of our sun (yellow is positive, light blue is negative). Red and blue represent weaker positive and negative magnetic fields, respectively. 

Video by Philipp Mösta

Read more: http://news.berkeley.edu/2015/11/30/missing-link-between-turbulence-hypernovae-and-gamma-ray-bursts/

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