Shinecon.org

 

 
 
Sessions
Chromospheric Connections to the Heliosphere
Connecting Solar and Heliospheric Physics during the Protracted Solar Minimum
Differential Emission Measure: Techniques and Implications
Extended Duration High-Energy Flares and GLEs
How Much do Solar Flares Contribute to Large SEP Events at Earth?
Imbalanced Turbulence in the Solar Wind
Magnetic Data as Drivers of Coronal Models: the Good, the Bad, and the Ugly
New Questions about Energetic Neutral Atoms, Pickup Ions, and Anomalous Cosmic Rays in the Heliosphere
Other
Physics-based “All Clear” Forecasting
Pinning Down the Physical Processes that Generate the Solar Wind
Progress and Challenges in Modeling a CME from its Eruption to its Interplanetary Propagation out past Earth: The May 13, 2005 Event
SDO Data Analysis How-To
The Nature of Coronal Mass Ejections: Heliospheric Properties and Relation to In-Situ Properties
Understanding and Predicting the Solar Cycle
When and How is Reconnection in the Solar Environment Turbulent?
 

 

     



SHINE 2010 Participants

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2010 SHINE Abstracts

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