File:PIA19822-MagneticBlackHoleWaves-AlfvenS-waves-20150709.jpg

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Summary

PIA19822: Magnetic Black Hole Waves

<a rel="nofollow" class="external free" href="http://photojournal.jpl.nasa.gov/catalog/PIA19822">http://photojournal.jpl.nasa.gov/catalog/PIA19822</a>

This cartoon shows how magnetic waves, called Alfven S-waves, propagate outward from the base of black hole jets. The jet is a flow of charged particles, called a plasma, which is launched by a black hole. The jet has a helical magnetic field (yellow coil) permeating the plasma. The waves then travel along the jet, in the direction of the plasma flow, but at a velocity determined by both the jet's magnetic properties and the plasma flow speed. The BL Lac jet examined in a new study is several light-years long, and the wave speed is about 98 percent the speed of light.

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current17:28, 5 January 2017Thumbnail for version as of 17:28, 5 January 20171,000 × 1,250 (180 KB)127.0.0.1 (talk)PIA19822: Magnetic Black Hole Waves <p><a rel="nofollow" class="external free" href="http://photojournal.jpl.nasa.gov/catalog/PIA19822">http://photojournal.jpl.nasa.gov/catalog/PIA19822</a> </p> This cartoon shows how magnetic waves, called Alfven S-waves, propagate outward from the base of black hole jets. The jet is a flow of charged particles, called a plasma, which is launched by a black hole. The jet has a helical magnetic field (yellow coil) permeating the plasma. The waves then travel along the jet, in the direction of the plasma flow, but at a velocity determined by both the jet's magnetic properties and the plasma flow speed. The BL Lac jet examined in a new study is several light-years long, and the wave speed is about 98 percent the speed of light.
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