SHINE Workshops Historical Archive
Home
Workshops
Locations
All SHINE Presentations
SHINE Website
Shock Geometry, Seed Populations, and the Origin of Energy-Dependent Fe/O in Large, Gradual Solar Energetic Particle Events (Tylka and Lee)
Written by
KTINDIANA
in
SHINE 2004
InvitedTylkaSHINE_Final_2004
Download
←
Electron Delays (HVC)
Magnetic Flux Ropes from the Sun to 1 AU (Jonathan Krall)
→
More posts
Working Group Summary: Special Session on the 2005 January 20 Event (Claire Foullon)
February 14, 2026
Plenary: Special Session on the 2005 January 20 Event (Allan Tylka)
February 14, 2026
RHESSI Observations of the 2005 January 20 Solar Flare (Gerald Share)
February 14, 2026
Jan 20, 2005 CME: Quasi-Parallel or Quasi-Perp? (J. Raymond)
February 14, 2026