Research Center for Astronomy

Events

Tuesday 19 December 2017 @ 12:00

A Review of Chaos in BQM

Athanasios C. Tzemos
Research Center for Astronomy and Applied Mathematics of the Academy of Athens


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Featured Picture

Numerical simulation of the axisymmetric ideal force-free pulsar magnetosphere.

Numerical simulation of the axisymmetric ideal force-free pulsar magnetosphere with Aristotelian dissipation in the current sheet (lines with arrows: poloidal magnetic field; color scale: poloidal electric current density; distances in units of the light cylinder radius). Only the equatorial current sheet survives beyond the light cylinder, as expected in Contopoulos, Kalapotharakos & Kazanas 2014, and seen very clearly in Cerutti, Philippov, Parfrey & Spitkovsky 2015 (adapted from Contopoulos 2016, "Are there two types of pulsars?", Monthly Notices, 463, L94).

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