Difference between revisions of "09/30/2012 23:00:00 UTC"
(→Video Data) |
(→In-Situ Data) |
||
| Line 11: | Line 11: | ||
[[File:plot_sw_vel_2012093000.png|350px]] <br /> | [[File:plot_sw_vel_2012093000.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. | ||
| + | |||
| + | ==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. | ||
| + | |||
| + | [[File:20120928stack.png]] <br> | ||
| + | |||
| + | 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 <br> | ||
==GOES X-RAY FLUX== | ==GOES X-RAY FLUX== | ||
Revision as of 15:05, 14 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
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
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
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.
