'Magnetic field generation' diaporamas de présentation

Physical Processes in Solar and Stellar Flares

Physical Processes in Solar and Stellar Flares. Eric Hilton. General Exam March 17th, 2008. Outline. Overview and Flare Observations Physical Processes on the Sun Standard Two-ribbon Model Magnetic Reconnection Particle Acceleration Stellar Comparison Summary. The Sun.

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Class 8: Jupiter, Saturn, Uranus, Neptune, Pluto

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Magnetosphere (magnetic field)

Magnetosphere (magnetic field). Convection of liquid metals in the outer core creates the Earth's magnetic field. Extends outward from the Earth for several thousand kilometers

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FilamenTATION INSTABILITIES IN RELATIVISTIC PLASMA

Almog Yalinewich. FilamenTATION INSTABILITIES IN RELATIVISTIC PLASMA. Introduction Theoretical background Numerical results Conclusions. Table of contents. GRBs are the most luminous flashes since the Big Bang They last between ~0.01 and ~100 seconds

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hubblesite/newscenter/archive/releases/2006/30/image/a/format/xlarge_web/

Particle Acceleration by Shocks. Tony Bell with Brian Reville, Klara Schure, Gwenael Giacinti University of Oxford. http://hubblesite.org/newscenter/archive/releases/2006/30/image/a/format/xlarge_web/. Cassiopeia A. Radio (VLA). Infrared (Spitzer). chandra.harvard.edu/photo/

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CRYOGENIC SPECTROMETER PROTOTYPE

CRYOGENIC SPECTROMETER PROTOTYPE. Rationale:

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Graduate Student Welcome Week September 2, 2014

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