Difference between revisions of "05/21/2007 21:00:00 UTC"
m (Phess4 moved page 05/19/2007 to 05/22/2007 02:00:00 UTC) |
|||
| Line 1: | Line 1: | ||
| − | + | =Comment Section= | |
| + | |||
| + | =Image Data= | ||
| + | ==In-Situ Data== | ||
| + | A combination of SWEPAM and MAG data from the ACE Satellite: <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 | *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 | ||
Revision as of 11:24, 1 July 2013
Comment Section
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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
