Difference between revisions of "03/08/2012 11:00:00 UTC"

From heliophysics
Jump to: navigation, search
(References)
(In-Situ Data)
Line 7: Line 7:
 
==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_2012030700.png|350px]]
+
[[File:plot_sw_mag_plasma_2012030800.png|350px]]
[[File:plot_sw_mag_2012030700.png|400px]]
+
[[File:plot_sw_mag_2012030800.png|400px]]
[[File:plot_sw_vel_2012030700.png|350px]] <br />
+
[[File:plot_sw_vel_2012030800.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 12:54, 2 July 2013

Comment Section

  • A fair ICME event, but strong solar source
    • X1 flare, fast CME, originated from the eastern hemisphere (~N18E42)
    • Solar wind plasma data is corrupted.

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.

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

  • Ying Liu et al. 2013 ApJ