03/30/2011 01:00:00 UTC

From heliophysics
Revision as of 05:13, 19 June 2013 by Moestlc (talk | contribs) (→‎Comment Section)
Jump to: navigation, search

Comment Section

  • A slow ICME with extremely long duration as seen at 1 AU
  • Seems an excellent example of the so-called "global" CME, or longitudinal extended CME (Jie)
    • COR2 A: symmetric above both east and west limbs along the equator, indicating a global feature
    • COR2 B: same as COR2, symmetric above both limbs
    • Combining COR2 A and B, it seems a global CME, surrounding the entire solar equator
    • Also a "stealth" CME: Need to check AIA and EUVI data to confirm the source
    • There is no apparent halo-like feature as seen from LASCO


  • Is the CME over-expanding (Gosling et al. )?


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.

GOES X-RAY FLUX

Error creating thumbnail: File missing



The GOES X-ray Flux of the flare associated with the event. The vertical line approximately denotes the flare peak time.

Video Data

References

Retrieved from "http://solar.gmu.edu/heliophysics/index.php?title=03/30/2011_01:00:00_UTC&oldid=1531"