SHINE 2013 Abstracts

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Sessions

Abundances in the solar atmosphere and in the solar wind
Campaign Event: The Extreme CME of 2012 July 23
Corotating Interaction Regions and the Connection Between Their Trailing Edges and Energetic Particle Acceleration Near 1 AU
Diagnostic of Chromospheric Flare Plasma
Identifying Coronal Holes in Solar Disk Observations
Interaction of CMEs with Coronal and Heliospheric Structures
Investigating the Origin of the Long-Duration High-Energy Gamma-Ray Flares
Mechanisms of Heavy Ion Heating in the In Situ Solar Wind
Observations of the Highest Energy Particles from the Sun and the Identification of their Acceleration Mechanism
Other
Plasma Turbulence at Fluid and Kinetic Scales
Turbulent Dissipation Challenge: Towards a convergence of current ideas
What do we learn from observations and modeling of the solar corona for understanding solar energetic particle events?
What Exactly is a Coronal Mass Ejection?
 
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