PPT-CH 8: Magnetic Fields

85 Applications of Electric and Magnetic Fields Agenda Quiz Lesson on Section on 85 Lots of Videos Story Time Cyclotron Particle Accelerator http wwwyoutubecomwatchvcNnNM2ZqIsc. Dayal Wickramasinghe and Lilia . Ferrario. Australian National University. Canberra. . . The chemically peculiar . Ap. , Bp stars ( ~ 1.8 -5 . M. sun. ) are magnetic, and . have ordered large. scale fields, . Poynting. dominated outflows. Yuri . Lyubarsky. Ben-Gurion . University . Ubiquity . of relativistic . outflows in astrophysics. Crab nebula in X-rays. M 87. GRB lightcurves. R. elativistic outflows are associated with: . a physical perspective . . 1. Philip Judge, . . High Altitude Observatory, NCAR. "Double, double, toil and trouble;. Fire burn, and cauldron bubble!". -- . . Alexei A. . Pevtsov. US National Solar Observatory. What is Space Climate Anyway?. SW–SC Similarities. Same drivers (solar eruptive events, open magnetic fields/CHs, solar wind). Similar spatial scales (quiet Sun, large-scale magnetic fields).. Amanda J. Fagan. Wittenberg University. March 19, 2014. Outline. Problem statement. Precession. Frequency. Sample Problem. Sources. Questions?. 2. Problem statement. a) Show that a spinning magnetic moment in the presence of a magnetic field leads to a precession of the magnetic moment. . Magnetic fields and nomenclature. Lorentz force: . . F . = q. v. . x . B. for which . q. v. . = flow of electronic charge = . Id. l. F. . = . Id. l. . x . B. . → . FBI rule. (left hand rule) defines the orientation relationship.. due to Currents . Chapter. 29. Copyright © 2014 John Wiley & Sons, Inc. All rights reserved.. 29-1. Magnetic Field due to a Current. 29.01 . Sketch a current-length element in a wire and indicate the direction of the magnetic field that it sets up at a given point near the wire.. basic concepts and magnetic topology . Anna (. Ania. ) . Malanushenko. Plasma. Is matter…. Mass is conserved. Momentum is conserved. Energy is conserved. …ionized and in magnetic field. Obeys Maxwell’s equations. Magnetic Forces. Objectives: . FLASHBACK. FLASHBACK: Sketch a stress-strain graph for a malleable materials and label a) the limit of proportionality b) the elastic limit c) the ultimate tensile strength d) the breaking point. at HIMAC synchrotron. Hiroshi Uchiyama . #,A). , Masahiro Kawashima . A). , . Shunsuke. Saito . A). , Izumi Kobayashi . A). , . Tadahiro. . Shiraishi. . A). ,. Chihiro. Kobayashi . A). , Eiichi . protostellar. cores?. Chat Hull. University of California, Berkeley (USA). Radio Astronomy Laboratory. 5. February 2013. Session: Magnetic Fields in the ISM and Star-forming Regions I. Magnetic Fields in the Universe IV. Systems. Frank Barnes.  . Department of Electrical, Computer, and Energy Engineering, University of Colorado, Boulder, Colorado. Acknowledgement. Ben Greenebaum. . Lucas Portelli . Carlos Martino . “. 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, . chiral magnetic effect. Fuqiang Wang. Purdue University. Strongly interacting matter in extreme magnetic fields. OUTLINE. Chiral magnetic effect (CME) and the. Dg. observable. Flow and nonflow backgrounds.