Difference between revisions of "Working Group 2"
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=='''Results of the Workshop and Future Plans'''== | =='''Results of the Workshop and Future Plans'''== | ||
Revision as of 03:06, 1 June 2013
Theory group led by Bojan Vrsnak (Croatia) and Yuming Wang (China)
Objectives
- Initiation of CMEs and their take-off dynamics ("acceleration stage")
- Heliospheric dynamics of ICMEs and evolution of their structure
- Relationship between empirical, analytical, and numerical propagation models and comparison with observations; forecasting aspects
- CME/ICME-associated phenomena (flares, shocks, etc.)
Scientific Questions
Which mechanisms, processes, forces are governing the CME take-off and ICME propagation?
2.1.1 What is the role of the flare-associated reconnection?
2.1.2 What is the role of emerging flux and poloidal-flux injection?
2.1.3 How long the Lorentz force dominates over the aerodynamic drag
2.1.4 How the inductive effects affect the CME eruption and ICME propagation?
2.1.5 What is the role of the ICME/ambient-field reconnection?
How much variable ambient conditions affect ICMEs?
2.2.1 Which processes are involved in ICME-ICME interactions?
2.2.2 How ICME-ICME interactions affect the dynamics and structure of ICMEs?
2.2.3 How high-speed solar wind streams (corotating interacting regions) affect ICMEs?
2.2.4 How the ICME-driven shock forms and evolves in the decreasing Alfven-velocity environment?
2.2.5 How ambient solar wind exchanges momentum, energy and magnetic flux with ICMEs?
What is the state of the art in the ICME-arrival and ICME-geoeffectiveness forecasting?
2.3.1 What are forecasting-performances of various empirical, analytical, and numerical models?
2.3.2 How well models reproduce heliospheric kinematics of ICMEs?
2.3.3 What are the key model-input parameters?
2.3.4 What can be done regarding the geoeffectiveness forecasting?
The CME-associated phenomena
2.4.1 What are the mechanisms of initiation and what is the nature of CME-driven coronal waves and shocks?
2.4.2 What is the role of flares in the initiation and acceleration of CMEs?
2.4.3 What can we learn from coronal dimmings?
2.4.4 How the associated phenomena (flares, waves, dimmings) can help in the space-weather forecasting?
2.4.5 How SEPs are accelerated by shocks and how they transport in heliosphere?
