Difference between revisions of "08/03/2010 16:00:00 UTC"
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| + | *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
Contents
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:
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The blue lines are an approximation of the CME cloud and the red line denotes the shock.
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
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
