Modeling 3-D Solar Wind Structure.pdf

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The CME will Interact with both the Slow Flow and the Fast Flow • Cuts at two latitudes – green lines.
The Interaction • As the CME passes through the streamer belt it decelerates. • Leading edge of the fast stream interacts with the slow streamer belt flow and forms a pair (forward and reverse) of shocks. • The CME is trapped between the fast coronal hole flow and the slow streamer belt – it is sandwiched with the CIR structure. • The CME effects the CIR evolution as well – the trailing CIR is eroded.
Page 1 and 2: Lecture 13 Modeling 3-D 3 D Solar W
Page 3 and 4: Enlil was the Sumarian Lord of the
Page 5 and 6: Formulation of ENLIL: Additional Co
Page 7: Launch a CME into the Streamer Belt
Page 11 and 12: A Slice Below the Equatorial Plane
Page 13 and 14: Source Surface Model and Velocity a
Page 15 and 16: Distribution of Solar Wind Paramete
Page 17 and 18: Visualization of Propagating CME
Page 19 and 20: Effect of Time Dependent Solar Mode
Page 21 and 22: Results at Other Locations at 1AU -

Modeling 3-D Solar Wind Structure.pdf

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