Difference between revisions of "05/21/2007 21:00:00 UTC"

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(In-Situ Data)
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==In-Situ Data==
 
==In-Situ Data==
 
A combination of SWEPAM and MAG data from the ACE Satellite: <br />
 
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.
 
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
  

Revision as of 13:17, 1 July 2013

Comment Section

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.

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