Difference between revisions of "07/14/2012 17:00:00 UTC"

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(In-Situ Data)
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[[File:plot_sw_mag_2012071400.png|400px]]
 
[[File:plot_sw_mag_2012071400.png|400px]]
 
[[File:plot_sw_vel_2012071400.png|350px]] <br />
 
[[File:plot_sw_vel_2012071400.png|350px]] <br />
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.<br />
[[File:eve_flare_2012_07_12.pdf]]
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[[File:eve_flare_2012_07_12.pdf]] EVE and GOES flare profiles
  
 
==GOES X-RAY FLUX==
 
==GOES X-RAY FLUX==

Revision as of 01:18, 7 June 2013

Comment Section

  • A perfect CME-ICME chain event (J. Zhang)
    • classical ICME feature: shock + sheath + magnetic cloud
    • strong solar signature: X1 flare (S17W08); halo CME, fast and bright
  • Propagation Direction is very close to the Sun Earth Line, making this a good event for comparing observations nearer the Sun to in-situ signatures (P. Hess)

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.
File:Eve flare 2012 07 12.pdf EVE and GOES flare profiles

GOES X-RAY FLUX

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

Video Data

COR2A
COR2B
HI1A
HI1B
HI2A
HI2B