'Mhd simulations' diaporamas de présentation

X-rays from Magnetically Channeled Winds of OB Stars

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X-rays from Magnetically Channeled Winds of OB Stars

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MHD simulations on eruption triggered by flux emergence

FEW2011 2011.8.22-25 Berkeley, USA. MHD simulations on eruption triggered by flux emergence. T. Yokoyama University of Tokyo Collaborators K. Nagashima (Stanford U.), S. Notoya, T. Kaneko (U. Tokyo) Based on the papers Notoya, 2006, master degree thesis, U. Tokyo

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Modeling Supercritical Accretion Flow Shin Mineshige (Kyoto) & Ken Ohsuga (RIKEN)

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Formation des filaments dans le milieu interstellaire

Formation des filaments dans le milieu interstellaire. Patrick Hennebelle. Molecular clouds and Map of spectra. Hily-Blant & Falgarone. Structure functions in molecular clouds (Hily-Blant et al. 2008). Polaris (Kosmas). Taurus (IRAM). Polaris (IRAM). S p. S 3. SL94. K41.

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MHD Simulations of Flux Cancellation on the Sun*

MHD Simulations of Flux Cancellation on the Sun*. Judy Karpen, Spiro Antiochos, Rick DeVore, and Mark Linton. *Work supported by ONR and NASA. Outline. What is flux cancellation? Origins Methodology Results Conclusions Questions. What is Flux Cancellation?.

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Beno i t Lavraud CESR/CNRS, Toulouse, France Uppsala, May 2008

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Solar MURI Vector Magnetogram Mini-Workshop

Solar MURI Vector Magnetogram Mini-Workshop. Using Vector Magnetograms in Theoretical Models: Plan of Action. Overview of the plan. Phase I Analyze available data for 1998 May 1 event Construct coronal magnetic equilibria Develop velocity inversion methods Test velocity inversion methods

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Magnetic Reconnection in Plasma

Magnetic Reconnection in Plasma. Plasmoid Generation and Dynamics Ravi Samtaney PSE and MCSE Divisions, KAUST. Motivation. Solar flares and Coronal Mass Ejections arise because the magnetic field lines in the Sun break and rejoin in a different configuration . . Other areas

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