Interplay between Kelvin-Helmholtz and urrent-driven instabilities in jets
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منابع مشابه
The Role of Macroscopic and Microscopic Jet Instabilities
Relativistic jets, be they Poynting flux or kinetic flux dominated, are current driven (CD) and/or Kelvin-Helmholtz (KH) velocity shear driven unstable. These macroscopic MHD instabilities may be responsible for some of the observed larger scale twisted jet structures and typically do not disrupt jets on less than kiloparsec scales. Here I review our understanding of the jet properties that wil...
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