Download presentation
Presentation is loading. Please wait.
Published byShon Derek Parker Modified over 6 years ago
1
Understanding the Structure and Morphology of Coronal Mass Ejections by Integrating Observations and Modeling Scene Setting Talks: Miho Janvier (IAS) & Ben Lynch (UCB) Monday (1 of 3): 1400, Aspen Room - How Good Are the In-Situ Observations of 3D CME / Interplanetary CME Flux Ropes? - Linking the Solar Source Structures of CMEs and Their Interplanetary Observations Organizers: M. Janvier (IAS), T. Nieves-Chinchilla (CUA), W. Manchester (UMich), M. Linton (NRL) SHINE Liaison: N. Lugaz (UNH)
2
Monday (2 of 3): 1545, Aspen Room
- 3D Flux Rope Orientation From Corona and Inner Heliosphere Observations and From Modeling How well do they match? Statistically? Event-by-event? How do we combine with numerical MHD simulations? Thursday (3 of 3): 1400, Aspen Room - Observations + Modeling + Simulations of ICME Propagation & Evolution How can different techniques be integrated to obtain evolution of ICMEs? Future Progress: Case studies versus generic models? What are the most important physics?
Similar presentations
© 2025 SlidePlayer.com. Inc.
All rights reserved.