Difference between revisions of "01/26/2009 05:00:00 UTC"
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=Comment Section= | =Comment Section= | ||
| + | *Can this short-duration event be classified as an ICME? (Jie) | ||
| + | **If yes, what is the source CME on the Sun? I can not find any possible source from C2 or COR2 | ||
| + | **If no, why the structure of enhanced magnetic field and enhanced density? | ||
=Image Data= | =Image Data= | ||
| + | ==In-Situ Data== | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2009012500.png|350px]] | ||
| + | [[File:plot_sw_mag_2009012500.png|400px]] | ||
| + | [[File:plot_sw_vel_2009012500.png|350px]] <br /> | ||
| + | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
=Video Data= | =Video Data= | ||
| + | |||
| + | =References= | ||
Latest revision as of 03:28, 19 June 2013
Comment Section
- Can this short-duration event be classified as an ICME? (Jie)
- If yes, what is the source CME on the Sun? I can not find any possible source from C2 or COR2
- If no, why the structure of enhanced magnetic field and enhanced density?
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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Error creating thumbnail: File missing
Error creating thumbnail: File missing
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
