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(add entry on the magnetorotational instability)
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Let us consider two close concentric rings in an accretion disc, such that the difference in radii is much smaller than the average radius <math> r \gg \Delta r </math>. In isolation, each ring would rotate at a slightly different Keplerian rate <math> \approx \Omega_k </math>. If the accretion disc is fully ionised, then the ambient magnetic field will act like a spring, trying to synchronise the two rings. The rate at which the magnetic field transfers energy and momentum is the Alfven velocity divided by the radius difference <math> V_A / \Delta r </math>. When this rate is smaller than the Keplerian frequency, then the accretion disc winds up the magnetic field lines and amplifies them.
 
Let us consider two close concentric rings in an accretion disc, such that the difference in radii is much smaller than the average radius <math> r \gg \Delta r </math>. In isolation, each ring would rotate at a slightly different Keplerian rate <math> \approx \Omega_k </math>. If the accretion disc is fully ionised, then the ambient magnetic field will act like a spring, trying to synchronise the two rings. The rate at which the magnetic field transfers energy and momentum is the Alfven velocity divided by the radius difference <math> V_A / \Delta r </math>. When this rate is smaller than the Keplerian frequency, then the accretion disc winds up the magnetic field lines and amplifies them.
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[[Category:Plasma physics]]

Revision as of 10:47, 31 October 2017

Let us consider two close concentric rings in an accretion disc, such that the difference in radii is much smaller than the average radius . In isolation, each ring would rotate at a slightly different Keplerian rate . If the accretion disc is fully ionised, then the ambient magnetic field will act like a spring, trying to synchronise the two rings. The rate at which the magnetic field transfers energy and momentum is the Alfven velocity divided by the radius difference . When this rate is smaller than the Keplerian frequency, then the accretion disc winds up the magnetic field lines and amplifies them.