SHINE Workshops Historical Archive
Home
Workshops
Locations
All SHINE Presentations
SHINE Website
Modeling particle acceleration at CME-driven shock and transport in the inner heliosphere, A case study (Gang Li)
Written by
KTINDIANA
in
SHINE 2004
gang_li-Shine-2004
Download
←
Dimmings & Related X-Ray Structures Following CME Onset (Forbes)
Shock Acceleration (Joe Giacalone)
→
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