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Introduction. 1. Magnetic Reconnection as a Heating Mechanism for the X-Ray Emitting Flare Loops and for Slow Coronal Transients. 2. The Neutral High-Temperature Turbulent Current Sheet. 3. The High-Temperature Turbulent Current Sheet with a Small Transverse Magnetic Field. 4. The Current Sheet Structure under the Fast and Slow Reconnection Regimes. 5. The Effect of Longitudinal Magnetic Field in the Current Sheets on the Sun. Conclusions. References. Index.
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Hunter Zickrick
reviewed Physical Processes In Solar Flares on September 02, 2011
Physical Processes In Solar Flares
Grey skies are gonna CLEAR UP! So put on a happy face!
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Add Physical Processes In Solar Flares, Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of te, Physical Processes In Solar Flares to the inventory that you are selling on WonderClubX
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Add Physical Processes In Solar Flares, Solar flares are very complex electromagnetic phenomena of a cataclysmic nature. Particles are accelerated to very high velocities and a variety of physical processes happen inside and outside flares. These processes can be studied by a large number of te, Physical Processes In Solar Flares to your collection on WonderClub |
