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| + | Partially due to the location of the spacecraft perhaps, I cannot see anything in STEREO to cause. I also see no significant Halo CMEs in LASCO during the days leading up to the in-situ signature | ||
=Image Data= | =Image Data= | ||
Revision as of 10:53, 9 July 2013
Comment Section
Partially due to the location of the spacecraft perhaps, I cannot see anything in STEREO to cause. I also see no significant Halo CMEs in LASCO during the days leading up to the in-situ signature
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
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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
