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SHINE 2005
Presentations and media associated with SHINE 2005
How particles are accelerated to high energies in large SEP events? (Gang Li)
SHINE_Li_2005
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January 5, 2026
End to End Modeling: The Community Coordinated Modeling Center Perspective (Peter MacNeice)
SHINE_McNiece_2005
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January 5, 2026
Finite-Time Shock Acceleration and Fits to ESP Ion Spectra (Chanruangrith Channok, David Ruffolo)
SHINE_Ruffolo_2005
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January 5, 2026
Solar Energetic Particles: Acceleration and Transport in Realistic Magnetic Fields (Igor Sokolov)
SHINE_Sokolov_2005
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January 5, 2026
Coupling Frameworks in Solar-Terrestrial Research (Chuck Goodrich)
STRcoupling_Goodrich_2005
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January 5, 2026
Progress and Challenges Towards Data- Driven CME Modeling: 2003 Oct 28 Event (Ilia Roussev)
SHINE05_Ilia_CME_modeling
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January 5, 2026
The Role of Sub-Surface Processes in the Formation of Coronal Magnetic Flux Ropes (A. A. van Ballegooijen)
shine05_Ballegooijen
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January 5, 2026
The Source of Magnetic Shear That Drives CMEs (Ward Manchester)
SHINEshear_Chip_2005
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January 5, 2026
Local Helioseismic Inferences of Sub-surface Magnetism and Dynamics (Doug Braun)
dbraun_05_shine
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January 5, 2026
Plenary: The Importance of Sub-surface Magnetic Field Structure and Evolution (George H. Fisher)
plenary-interior_Fisher_2005
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January 5, 2026
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