Construct · 2 fields · 2 citations
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In optics, collimation is the process of making a beam's rays parallel, so that the beam neither converges nor spreads appreciably with distance: a point source placed at the focal point of a lens or mirror emerges collimated. Jenkins and White's Fundamentals of optics treats the geometry; in practice perfect collimation is limited by the finite source size and by diffraction. The referent is a beam held to near-parallel propagation, and the key quantity is how little it diverges.[1]
In astrophysics, collimation is the confinement of an outflow (a protostellar or active-galactic-nucleus jet) into a narrow, nearly parallel beam that stays focused over distances vast compared with its width. Blandford and Payne's 1982 Hydromagnetic flows from accretion discs and the production of radio jets showed how magnetic forces anchored in the accretion disc can launch and collimate such jets. It is the same parallel-beam construct as collimated light, here realised in a magnetised plasma outflow and measured by the jet's opening angle.[2]
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