Numerical Simulations of iCMEs and Comparison with Heliospheric Images
Abstract
CONCLUSION: Simulations are an important tool in support of HI observations * For complex events (CME-CME interaction): What happened? Testing different physical mechanisms * To test and validate methods: Simulations are like a controlled laboratory environment: CME speed and direction are known, Can vary only one parameter. We tested the Fixed-Phi and Point-P approximations. We devised a new approximation which fits better our simulated CME and is important at large elongation angles (beyond 40-deg). Lack of fast/wide CMEs may explain why fitting method work so well so far.
Document Details
- Document Type
- Technical Report
- Publication Date
- May 06, 2010
- Accession Number
- ADA526882
Entities
People
- Angelos Vourlidas
- Ilia Roussev
- Noe Lugaz
- T. Gombosi
- W. Manchester
Organizations
- University of Hawaiʻi System