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The inner knot of the Crab nebula
Maxim Lyutikov, Serguei Komissarov, Oliver Porth
We model the inner knot of the Crab Nebula as a synchrotron emission coming from the non-spherical MHD termination shock of relativistic pulsar wind. The post-shock flow is mildly…
Solar prominences: 'double, double ... boil and bubble'
Rony Keppens, Chun Xia, Oliver Porth
Observations revealed rich dynamics within prominences, the cool 10,000 K, macroscopic (sizes of order 100 Mm) "clouds" in the million degree solar corona. Even quiescent prominenc…
Stationary Relativistic Jets
S. S. Komissarov, O. Porth, M. Lyutikov
In this paper we describe a simple numerical approach which allows to study the structure of steady-state axisymmetric relativistic jets using one-dimensional time-dependent simula…