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toward a Maxwellian distribution Maxwellians have special properties that make them simpleto use but plasmas are not always Maxwellian Thus one must be very careful about applyingtheories or equa. In addition magnetic fields create a force only on moving charges The direction the magnetic field produced by a moving charge is perpendicular to the direction of motion The direction of the force due to a magnetic field is perpendicular to the dir David Cohen. Swarthmore College. If we understand the physical connection between magnetic fields in massive stars and X-rays, we could use X-ray observations to identify magnetic massive stars.. e.g. Which of the stars in this Chandra X-ray image of the Orion Nebula Cluster are massive magnetic stars? . 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. 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, . Bob Merlino. Plasma Seminar. April 13, 2015. 1. Background. The MDPX is an dusty plasma device at Auburn University (AL) designed to study dusty plasmas in magnetic fields up to 4 T.. D. iscussions began in . 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. RIKEN-BNL . Research Center. Nonlinear QED effects on photon and . dilepton. spectra . in . supercritical . magnetic fields. KH. , K. . Itakura. (KEK), . Ann. . Phys. 330 (. 2013); Ann. Phys. 334 . Bob Merlino. Plasma Seminar. April 13, 2015. 1. Background. The MDPX is an dusty plasma device at Auburn University (AL) designed to study dusty plasmas in magnetic fields up to 4 T.. D. iscussions began in . 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. David Cohen. Swarthmore College. XMM-Newton. Chandra. Launched 2000: superior . sensitivity, . spatial resolution, and . spectral resolution. sub-. arcsecond. resolution. XMM-Newton. Chandra. Both have CCD detectors for imaging spectroscopy:. David Cohen. Swarthmore College. If we understand . the physical connection between magnetic fields in massive stars and X-rays, we could use X-ray observations to identify magnetic massive stars.. e.g. Which of the stars in this Chandra X-ray image of the Orion Nebula Cluster are massive magnetic stars? . Systems. Frank Barnes.  . Department of Electrical, Computer, and Energy Engineering, University of Colorado, Boulder, Colorado. Acknowledgement. Ben Greenebaum. . Lucas Portelli . Carlos Martino . Open: Venus – solar wind. Closed: Venus – Venus. Draped: solar wind – solar wind. Magnetic fields guide ion and electron motions. The connectivity (topology) of these field lines helps us to understand how the upper atmosphere interacts with the solar wind.. Presented by. Rick Lee. Chief Operator, DIII-D Operations. Manager, Energy/Fusion Outreach Program. General Atomics. San Diego, CA. “Tell me and I forget. Teach me and I remember. Involve me and I learn.” – Benjamin Franklin.