Titlebook: Energy Conversion and Particle Acceleration in the Solar Corona; Karl-Ludwig Klein Book 2003 Springer-Verlag Berlin Heidelberg 2003 Chromo

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Radio Diagnostics of Flare Energy Releasehe electrons. Less known are radio emissions from trapped electrons driving loss-cone unstable waves. This is the interpretation usually given to decimetric type IV emission. These types of coherent radio emission give clues on the geometry and plasma parameters near the acceleration region..More sp

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How Well Do We Understand Magnetic Reconnection?vestigation. While energetic electrons may be generated by the runaway effect in the diffusion region, any super-Alfvénic ions seem to be due to some mechanism not related directly to the reconnection process.

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What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations?es of 100 ms or less, even after particle transport effects have been considered. Millimeter wave observations also reveal spatial fragmentation. Together with distributions of overall event size, such fragmentation suggests a scale-invariant energy release process, such as would occur in a state of

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Transport of Energy from the Corona to the Chromosphere During Flaresresolved HXR observations (RHESSI) made simultaneously with a high-cadence detection of selected optical lines, one should be able to diagnose the properties of particle beams, provided that the response of the lower atmospheric layers to beam pulses is strong enough.

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Acceleration and Propagation of Solar Energetic Particleslar atmosphere. The comparison of interacting and escaping particles can provide valuable information about the question whether there is one dominant energization process in solar events, or whether particles are accelerated in multiple processes or sites. Equally important, the study of the propag

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Energy Conversion and Particle Acceleration in the Solar Corona

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