'Poynting flux' presentation slideshows

Cusp Type Configurations and Particle Energization

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Great Debate on GRB Composition: A Case for Poynting Flux Dominated GRB Jets

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ASTROPHYSICAL JETS

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The Magnetorotational Instability

The Magnetorotational Instability. 16 October 2004 Large Scale Computation in Astrophysics John F. Hawley University of Virginia. Jean-Pierre De Villiers (UVa; U. Calgary) Steven A. Balbus (UVa) Julian H. Krolik, Shigenobu Hirose (JHU) Charles F. Gammie (Illinois). Collaborators:.

477 views • 32 slides

General Relativistic MHD Simulations of Black Hole Accretion Disks

General Relativistic MHD Simulations of Black Hole Accretion Disks. John F. Hawley University of Virginia Presented at the conference on Ultra-relativistic Jets in Astrophysics Banff, July 12, 2005. Jean-Pierre De Villiers (U. Calgary) Steven A. Balbus (UVa, ENS)

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Comoving Acceleration by Relativistic Poynting Flux Edison Liang Rice University

Comoving Acceleration by Relativistic Poynting Flux Edison Liang Rice University Acknowledgements: Kasumi Nishimura, Koichi Noguchi (Japan); Peter Gary, Hui Li (LANL); Scott Wilks, Bruce Langdon (LLNL) Krakow, PL 2008. Side Note Nonlinear collective processes

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Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi

Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi Shinya Sugiyama, Rice University Acknowledgements: Scott Wilks, Bruce Langdon Bruce Remington Talk given at Glast Symposium 2007 (see http://spacibm.rice.edu/~liang/picsim and spacibm.rice.edu/~knoguchi ).

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Reconnection in the Magnetotail and the Solar Corona

Reconnection in the Magnetotail and the Solar Corona. J. Birn, M. Hesse Ackn.: R. Nakamura, E. Panov. photo: M.Hesse. Reconnection in the Magnetotail and the Solar Corona. Overview Bouncing and vortex flows Role of entropy loss/reduction Energetic particle fluxes (test electrons)

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Free magnetic energy is the difference between the energy of a given

B. T. Welsch (welsch@ssl.berkeley.edu) Space Sciences Lab, Univ. of California, Berkeley, CA 94720-7450 J. M. McTiernan (jimm@ssl.berkeley.edu) Space Sciences Lab, Univ. of California, Berkeley, CA 94720-7450 T. R. Metcalf (metcalf@cora.nwra.edu) NWRA, 3380 Mitchell Ln, Boulder, CO 80301

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Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi

Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi Shinya Sugiyama, Rice University Acknowledgements: Scott Wilks, Bruce Langdon Bruce Remington Talk given at Glast Symposium, Feb 2007 (see http://spacibm.rice.edu/~liang/picsim

312 views • 22 slides

Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi

Radiation from Poynting Jets and Collisionless Shocks Edison Liang, Koichi Noguchi Shinya Sugiyama, Rice University Acknowledgements: Scott Wilks, Bruce Langdon Bruce Remington Talk given at Glast Symposium, Feb 2007 (see http://spacibm.rice.edu/~liang/picsim

305 views • 22 slides

Magnetic Fields and Jet Formation

Magnetic Fields and Jet Formation. John F. Hawley University of Virginia Workshop on MRI Turbulence June 18 th 2008. Kris Beckwith (UVa) Julian H. Krolik (JHU) Scott Noble (JHU) Jake Simon (UVa). Collaborators :. Jet Formation. Young stellar objects

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I . V . Golovchanskaya , ?. V . Mingalev , ?. N . Melnik , B . V . Kozelov

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Hamrin, M., Norqvist, P., Marghitu, O., et al. e-mail: hamrin@space.umu.se

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ALFVEN WAVE ENERGY TRANSPORT IN SOLAR FLARES

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Importance of the Height Distribution of Joule Heating for Thermospheric Density

Importance of the Height Distribution of Joule Heating for Thermospheric Density Arthur D. Richmond and Astrid Maute NCAR High Altitude Observatory. . b. Field-Aligned Poynting Flux, IMF B z = -5 nT, B y = 0. S p|| . b. . b. Summer. 104 GW. 73 GW. 177 GW. 10. 10. 20. mW/m 2.

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