Solar and Interplanetary Dynamics (Symposium Summary)
How does the medium in between the sun and the earth and beyond the earth’s orbit, the socalled heliosphere, look like? Does a basic undisturbed heliosphere actually exist, and is one able to model its observed magnetic structures and plasma motions with their spatial and temporal variations?
How and where in the solar atmosphere are the disturbances generated and what are the characteristic time scales, geometries and energies involved?
KeywordsCurrent Sheet Coronal Hole Magnetic Reconnection Solar Atmosphere Interplanetary Medium
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