Difference between revisions of "07/14/2012 17:00:00 UTC"
(→Image Data) |
(→Image Data) |
||
| Line 15: | Line 15: | ||
== Heliospheric Imaging == | == Heliospheric Imaging == | ||
| − | + | CME track observed in Jmap with SATPLOT software (STEREO-A): | |
| − | [[File: | + | [[File:satplot_jmap_july122012.png|300px]]] |
| − | [[File: | + | results of geometrical modeling: |
| + | [[File:Geometry_12_july2012.jpeg|300px]]] | ||
==Flare Data== | ==Flare Data== | ||
Revision as of 04:10, 12 June 2013
Contents
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:
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.
Heliospheric Imaging
CME track observed in Jmap with SATPLOT software (STEREO-A):
Error creating thumbnail: File missing
]
results of geometrical modeling:
Error creating thumbnail: File missing
]
Flare Data
- File:Eve flare 2012 07 12.pdf EVE and GOES flare profiles
- 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.
