'Current sheets' diaporamas de présentation

Sarah Gibson

Sigmoids, filaments and cavities: how do they connect?. January 2006. Sarah Gibson. MOTIVATION:. Sigmoids, filaments, and cavities are of interest because of their observed connections to CMEs because they tell us about coronal equilibrium magnetic structures. OUTLINE. Brief review

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In situ observations of magnetic reconnection in solar system plasma

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Ilya Silin

Anomalous resistivity due to lower-hybrid drift waves. Results of Vlasov-code simulations and Cluster observations. Ilya Silin. Department of Physics University of Alberta isilin@phys.ualberta.ca.

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Pre-flare Energy Storage

Pre-flare Energy Storage. Dana Longcope Montana State University. The possible role of equilibrium current sheets. Thanks: Dave McKenzie Jonathan Cirtain Jason Scott. Work supported by NASA NAG5-10489. The Photospheric Field. 2001-08-10 12:51 UT. 2001-08-11 17:39 UT.

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Electron Energization and Radiation in MRI-driven Accretion Edison Liang, Rice University

Electron Energization and Radiation in MRI-driven Accretion Edison Liang, Rice University Collaborators: G. Hilburn, Rice; S. Liu, H. Li, LANL; C. Gammie, UI; M. Boettcher, Ohio U. DPP talk November 2008. High-energy emission of LLBH such as SgrA* examplifies

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The Structure of Thin Current Sheets Associated with Reconnection X-lines

The Structure of Thin Current Sheets Associated with Reconnection X-lines. Marc Swisdak The Second Workshop on Thin Current Sheets April 20, 2004. Collaborators. U. of Maryland. J. Drake M. Shay J. McIlhargey B. Rogers A. Zeiler. UMBC. Dartmouth College. MPP-Garching. z. y. x.

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Studying Solar Wind Magnetic Reconnection Events using Cluster.

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Magnetic Reconnection Across the HCS

Magnetic Reconnection Across the HCS. Mark Moldwin UM and Megan Cartwright UC-Berkeley. Isradynamics April 2010. With thanks to Mark Linton at NRL Linton and Moldwin, JGR, 2009. Cambridge Univ Press, 2009. Goal of Talk.

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Multiple Sheet Beam Instability of Current Sheets in Striped Relativistic Winds Jonathan Arons

Multiple Sheet Beam Instability of Current Sheets in Striped Relativistic Winds Jonathan Arons University of California, Berkeley. 1. latitude sector. As if energy flux. in a narrow. Crab Vela. G54.1 J2229.

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Evolution of understanding of solar wind-gaseous obstacle interaction O. Vaisberg Space Research Institute (IKI), Moscow

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STEREO Science Team Meeting February 2009 Marriott Hotel, Pasadena, CA

Physics of Dust Pickup in the Solar Wind: Contributions by STEREO C.T. Russell, L.K. Jian , J.G. Luhmann , D.R. Weimer. STEREO Science Team Meeting February 2009 Marriott Hotel, Pasadena, CA. Conventional Wisdom about Dust Pickup in Solar Wind.

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Cluster Workshop VI, 1-3 October, 2003 ESTEC

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ASYMMETRIC THIN CURRENT SHEETS: A 1-D TEST PARTICLE MODEL AND COMPARISON WITH SW DATA

ASYMMETRIC THIN CURRENT SHEETS: A 1-D TEST PARTICLE MODEL AND COMPARISON WITH SW DATA. J. Chen 1 and R. A. Santoro 2 1 Plasma Physics Division, Naval Research Laboratory 2 Lockheed Martin Management and Data System. The Second Workshop on Thin Current Sheets

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Hahn-Meitner-Institut Berlin

KH. Hahn-Meitner-Institut Berlin. Hahn-Meitner-Institut Berlin. Larmor phase corrections in neutron resonance spin-echo: curved dispersion surfaces. NMI3 General Meeting - Joint Research Activity Polarized Neutron Techniques, Task 2-A. Klaus Habicht Hahn-Meitner-Institut Berlin.

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Joule Heating and Anomalous Resistivity in the Solar Corona

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New STEREO/SECCHI Processing for Heliospheric Transients

New STEREO/SECCHI Processing for Heliospheric Transients. David F. Webb ISR, Boston College, MA, USA david.webb@bc.edu. New England Space Science Consortium meeting UNH, NH 24 October 2012. OUTLINE - BACKGROUND.

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The Role of Magnetic Geometry and Reconnection in the Origin of the Solar Wind

313 views • 9 slides

Dissipation of Solar Wind Turbulence

Dissipation of Solar Wind Turbulence. Thursday AM, Thursday PM, Friday AM John Podesta , Bill Matthaeus and Greg Howes. Dissipation of solar wind turbulence. Thursday Morning : Solar wind theory (1) Ben Chandran Thursday Afternoon: SW observations (1) Chuck Smith

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