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1. Introduction: The High-energy Corona – Waves, Eruptions, Particles

2. What Can Be Learned About Competing Acceleration Models from Multiwavelength Observations?

3. Particle Acceleration at the Earth’s Bow Shock

4. Pulsating Solar Radio Emission

5. Energetic Particles Related with Coronal and Interplanetary Shocks

6. Quasi-periodic Pulsations as a Diagnostic Tool for Coronal Plasma Parameters

7. Review of Selected RHESSI Solar Results

8. On the Existence of Non-maxwellian Velocity Distribution Functions in the Corona and their Consequences for the Solar Wind Acceleration

9. Recent Research: Large-scale Disturbances, their Origin and Consequences

10. Large-scale Waves and Shocks in the Solar Corona

11. Small Scale Energy Release and the Acceleration and Transport of Energetic Particles

12. RHESSI Results – Time for a Rethink?

13. Magnetic Complexity, Fragmentation, Particle Acceleration and Radio Emission from the Sun

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