Difference between revisions of "09/30/2012 23:00:00 UTC"
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**strong B | **strong B | ||
**possibly multiple CMEs interacting; need to check all halo CMEs in the plausible launch window | **possibly multiple CMEs interacting; need to check all halo CMEs in the plausible launch window | ||
| + | *C. Moestl: maybe two ICMEs, the shock of the 2nd travels through the first one | ||
| + | *simulations of these events? | ||
=Image Data= | =Image Data= | ||
Revision as of 02:44, 20 June 2013
Contents
Comment Section
- Complex ejecta at 1 AU (J. Zhang)
- strong B
- possibly multiple CMEs interacting; need to check all halo CMEs in the plausible launch window
- C. Moestl: maybe two ICMEs, the shock of the 2nd travels through the first one
- simulations of these events?
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.
Heliospheric Imaging
De-projected Height Time Plots of the shock and ejecta fronts as obtained from the GCS (measured by Hess) (for GCS details, see Thernisien 2006) along with velocity and acceleration profiles determined from the Aerodynamic Drag Model.
Fitting parameters in GCS Model: Carrington Longitude: 167.087 degrees, Latitude: 16.7706 degrees, Tilt Angle: -68.7582 degrees, Aspect Ratio: .326671, Half Angular Width: 33.2613
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
