PPT-Are magnetic fields and outflows aligned in

protostellar cores Chat Hull University of California Berkeley USA Radio Astronomy Laboratory 5 February 2013 Session Magnetic Fields in the ISM and Starforming Regions I Magnetic Fields in the Universe IV. Molecular Outflows in Low- and High-MassStar-forming RegionsH 8.5 – Applications of Electric and Magnetic Fields. Agenda. Quiz. Lesson on Section on 8.5. Lots of Video’s. Story Time. Cyclotron Particle Accelerator. http://. www.youtube.com/watch?v=cNnNM2ZqIsc. Andrii Neronov. University of Geneva. Durrer. & AN, . A&ARev. , 21, 62 (2013) . Overview . Magnetic fields in astronomy and cosmology. Characterization. of cosmological magnetic fields. Generation. outflows. : . 3C293 in 3D. Elizabeth . Mahony . (ASTRON, the Netherlands Institute for Radio Astronomy). Raffaella. . Morganti. (ASTRON, Univ. of Groningen). , Raymond . Oonk. (ASTRON). , Tom . Oosterloo. Yuri . Lyubarsky. Ben-Gurion University. Beer-. Sheva. , Israel . Universality of . relativistic jets. M 87. M 87. Crab in X-rays. GRBs. t. ime, s. t. ime, s. PKS 2155-304 . Pulsar magnetosphere. Christopher F. . McKee. MFU V Corsica. Oct 7, 2015. With: Pak-. Shing. Li. Richard Klein. IN STAR FORMATION. Partial support provided by the National Science Foundation and NASA. OUTLINE. III. Observing interstellar magnetic fields on a computer (LMK). Ashish. Myles. †. Nico. . Pietroni. * . Denis Kovacs. †. . Denis . Zorin. †. . †. . New York University. * . ISTI, Italian National Research Council. Motivation. Problem 1: . Convert. arbitrary meshes to . all magnets have magnetic poles – . . points at the ends of a magnet that have opposing magnetic qualities. all magnets have a north pole and south pole that are magnetically opposite. like poles repel and unlike poles attract. 21. History of Magnetism . In 1269, Pierre de Maricourt of France found that the directions of a needle near a spherical natural magnet formed lines that encircled the sphere and passed through two points diametrically opposite each other, which he called the poles of the magnet. Subsequent experiments showed that every magnet, regardless of its shape, has two poles, called North (N) and (S) poles, that exert forces on other magnetic poles similar to the way electric charges exert forces on one another. That is, like poles (N-N or S-S) repel each other, and opposite poles (N-S) attract each other. Crane Video. What do you know about magnetism?. Electricity and magnetism are related!. Modeling .  independent work  compare notes. Magnetism Readings. Turn and talk. …Partner closer to the door. Ashish. Myles. †. Nico. . Pietroni. * . Denis Kovacs. †. . Denis . Zorin. †. . †. . New York University. * . ISTI, Italian National Research Council. Motivation. Problem 1: . Convert. arbitrary meshes to . Ashish. Myles. †. Nico. . Pietroni. * . Denis Kovacs. †. . Denis . Zorin. †. . †. . New York University. * . ISTI, Italian National Research Council. Motivation. Problem 1: . Convert. arbitrary meshes to . “. Magnetic phases of spin-1 spin–orbit-coupled Bose . gases. ,”. D. L. Campbell, . R. . M. Price, . A. . Putra, . A. . Valdés-. Curiel. , . D. . . Trypogeorgos. , and.  I. B. . Spielman,. Nature Communications, . Seyfert. Galaxies Ark 564 and . Mrk. 590. Anjali. Gupta. Columbus State . Ohio State University. Collaborators: . Smita. . Mathur. , . Yair. . Krongold. Low velocity outflows are ubiquitous. .