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

From heliophysics
Jump to: navigation, search
(Comment Section)
(References)
 
(6 intermediate revisions by 4 users not shown)
Line 1: Line 1:
 
=Comment Section=
 
=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
+
*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]
 +
*A "well-behaved" CME-ICME event; clear eruption signature in EUV coronal images (Jie)
  
 
=Image Data=
 
=Image Data=
Line 9: Line 10:
 
[[File:plot_sw_vel_2010080300.png|350px]] <br />
 
[[File:plot_sw_vel_2010080300.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.
 +
 +
 +
==GOES X-RAY FLUX==
 +
[[File:20100801_goes.png|500px]]<br /><br />
 +
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)
 +
*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

Latest revision as of 11:31, 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