Difference between revisions of "08/03/2010 16:00:00 UTC"

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(Created page with "=Comment Section= =Image Data= =Video Data=")
 
(References)
 
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=Comment Section=
 
=Comment Section=
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*Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots, as well as some movies (STEREO); have a look under [http://www.uni-graz.at/igam-sophy/isest2013/20100801/ 2010-Aug-01 Events]
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*A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (Jie)
  
 
=Image Data=
 
=Image Data=
 +
==In-Situ Data==
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A combination of SWEPAM and MAG data from the ACE Satellite: <br />
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[[File:plot_sw_mag_plasma_2010080300.png|350px]]
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[[File:plot_sw_mag_2010080300.png|400px]]
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[[File:plot_sw_vel_2010080300.png|350px]] <br />
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
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 +
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==GOES X-RAY FLUX==
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[[File:20100801_goes.png|500px]]<br /><br />
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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. <br />
  
 
=Video Data=
 
=Video Data=
 +
 +
=References=
 +
*Harrison et al. 2012 ApJ (overview)
 +
*Liu et al. 2012 ApJ (interaction)
 +
*Odstrcil et al. 2013 JGR (simulation)
 +
*Temmer et al. 2012 ApJ (interaction)
 +
*Moestl et al. 2012 ApJ (in situ)
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*Webb et al. 2013 Sol. Phys. (HI, SMEI)
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*Martinez Oliveros 201? ApJ (radio)
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*Joshi and Srivastava 2010 and 2011 ApJ
 +
*Ting Li et al. 2011

Latest revision as of 12:31, 1 July 2013

Comment Section

  • Manuela Temmer: we can provide for close to the Sun deprojected height-time, velocity-time, acceleration-time, mass-time/distance plots, as well as some movies (STEREO); have a look under 2010-Aug-01 Events
  • A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (Jie)

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

  • Harrison et al. 2012 ApJ (overview)
  • Liu et al. 2012 ApJ (interaction)
  • Odstrcil et al. 2013 JGR (simulation)
  • Temmer et al. 2012 ApJ (interaction)
  • Moestl et al. 2012 ApJ (in situ)
  • Webb et al. 2013 Sol. Phys. (HI, SMEI)
  • Martinez Oliveros 201? ApJ (radio)
  • Joshi and Srivastava 2010 and 2011 ApJ
  • Ting Li et al. 2011