Difference between revisions of "05/21/2007 21:00:00 UTC"
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| − | + | =Comment Section= | |
| − | + | *Perhaps due to the location of the spacecraft, I cannot see anything in STEREO to cause the ICME. I also see no significant Halo CMEs in LASCO during the days leading up to the in-situ signature. The Ying Liu paper listed in the reference section dealt only with the in-situ data, so I am not sure about the CME connection for this event. (Hess) | |
| + | *Three density peaks seemed to correspond to (1) sector boundary, (2) small ejecta, and (3) CIR interface, respectively (Jie Zhang) | ||
| + | |||
| + | =Image Data= | ||
| + | ==In-Situ Data== | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
| + | [[File:plot_sw_mag_plasma_2007052000.png|350px]] | ||
| + | [[File:plot_sw_mag_2007052000.png|400px]] | ||
| + | [[File:plot_sw_vel_2007052000.png|350px]] <br /> | ||
| + | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
| + | |||
| + | =Video Data= | ||
| + | |||
| + | =References= | ||
| + | *compression of the magnetic cloud through a high speed stream (Rouillard et al. paper) | ||
| + | *Liu, Y., Luhmann, J. G., Huttunen, K. E. J., Lin, R. P., Bale, S. D., Russell, C. T., & Galvin, A. B. (2008). Reconstruction of the 2007 May 22 Magnetic Cloud: How Much Can We Trust the Flux-Rope Geometry of CMEs? Astrophysical Journal, 677(2), L133–L136. doi:10.1086/587839 | ||
Latest revision as of 23:20, 8 October 2016
Comment Section
- Perhaps due to the location of the spacecraft, I cannot see anything in STEREO to cause the ICME. I also see no significant Halo CMEs in LASCO during the days leading up to the in-situ signature. The Ying Liu paper listed in the reference section dealt only with the in-situ data, so I am not sure about the CME connection for this event. (Hess)
- Three density peaks seemed to correspond to (1) sector boundary, (2) small ejecta, and (3) CIR interface, respectively (Jie Zhang)
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
Error creating thumbnail: File missing
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.
Video Data
References
- compression of the magnetic cloud through a high speed stream (Rouillard et al. paper)
- Liu, Y., Luhmann, J. G., Huttunen, K. E. J., Lin, R. P., Bale, S. D., Russell, C. T., & Galvin, A. B. (2008). Reconstruction of the 2007 May 22 Magnetic Cloud: How Much Can We Trust the Flux-Rope Geometry of CMEs? Astrophysical Journal, 677(2), L133–L136. doi:10.1086/587839
