'Magneto-Spin' Effect Near Black Holes (7 of 9) (video) American Association for the Advancement of Science Share Print E-Mail Loading video... Caption Magneto-spin alignment effect simulation with rotating view: Spinning black hole (at center) produces a powerful jet (white-blue) along its spin axis. The jet affects the orientation of the surrounding accretion disk (infalling hot plasma as white-red near the hole) causing the disk to align with the spin axis near the hole, but at larger distances the disk dominates the jet and the jet re-aligns with the outer disk. This video relates to a paper that appeared in the Nov. 16, 2012, issue of Science, published by AAAS. The paper, by Jonathan C. McKinney at Stanford University in Stanford, Calif., and colleagues was titled, "'Magneto-Spin' Effect Near Black Holes." Credit Visualizations by Ralf Kaeler (KIPAC) and Jonathan McKinney (UMD) Usage Restrictions Please cite the owner of the video when publishing. This video may be freely used by reporters as part of news coverage, with proper attribution. Non-reporters must contact Science for permission. Share Print E-Mail Disclaimer: AAAS and EurekAlert! are not responsible for the accuracy of news releases posted to EurekAlert! by contributing institutions or for the use of any information through the EurekAlert system.