Modeling 3-D Solar Wind Structure.pdf
Modeling 3-D Solar Wind Structure.pdf
Modeling 3-D Solar Wind Structure.pdf
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A Slice Below the Equatorial Plane<br />
• The bottom panel show a<br />
time series at same<br />
colatitude at 3AU and<br />
fixed azimuth.<br />
• The shaded area<br />
indicates the CME<br />
material and the dotted<br />
line shows the injected<br />
number density profile.<br />
• The CME penetrates into<br />
the trailing region of the<br />
preceding fast stream.<br />
• The forward shock<br />
weakens and becomes a<br />
pressure wave.<br />
Forward Shock<br />
• The reverse shock forms at leading edge of CME and<br />
propagates backward through the CME material<br />
Reverse Shock
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