Cme acceleration - PowerPoint PPT Presentation

THEORY OF SOLAR MAGNETIC FLUX ROPES: CMEs DYNAMICS

THEORY OF SOLAR MAGNETIC FLUX ROPES: CMEs DYNAMICS. James Chen Plasma Physics Division, Naval Research Laboratory. George Mason University 21 Feb 2008. Canonical parameters of solar eruptions: KE, photons, particles erg Mass g Speed ~100 - 2000 km/s

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744 views • 42 slides

Properties of CME Acceleration in the Low Corona

SHINE June 28 – July 2, 2004 Big Sky - Montana. Properties of CME Acceleration in the Low Corona. Address the CME acceleration issue from the observational point of view: What? Duration Magnitude Distance

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443 views • 30 slides

ACCELERATION RESULTS

GOALS. 1.0. 1.0. 1.0. The two goals of this study are to examine the acceleration of CMEs in the low corona and to determine the most accurate CME start times in order to better understand the relationship between CMEs and other forms of solar activity, such as flares. 0.8. 0.8. 0.8. 0.6.

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113 views • 1 slides

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