Difference between revisions of "04/05/2010 08:00:00 UTC"
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=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 [http://www.uni-graz.at/igam-sophy/isest2013/20100403/ 2010-Apr-03 Event] | |
| + | * paper http://arxiv.org/abs/1110.0827 | ||
| + | *A well-behaved CME-ICME event (Jie) | ||
| + | *unsolved question: | ||
| + | explain the magnetic field profile of the ICME; | ||
| + | how well do predictions perform? | ||
=Image Data= | =Image Data= | ||
| Line 8: | Line 13: | ||
A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | A combination of SWEPAM and MAG data from the ACE Satellite: <br /> | ||
[[File:plot_sw_mag_plasma_2010040400.png|350px]] | [[File:plot_sw_mag_plasma_2010040400.png|350px]] | ||
| − | [[File:plot_sw_mag_2010040400.png| | + | [[File:plot_sw_mag_2010040400.png|400px]] |
| − | [[File:plot_sw_vel_2010040400.png|350px]] | + | [[File:plot_sw_vel_2010040400.png|350px]] <br /> |
| + | The blue lines are an approximation of the CME cloud and the red line denotes the shock. | ||
| − | == | + | ==Heliospheric Imaging== |
Jmaps from STEREO A and B along the CME leading edge position angle <br /> | Jmaps from STEREO A and B along the CME leading edge position angle <br /> | ||
[[File:jmapA20100403.png|500px]] | [[File:jmapA20100403.png|500px]] | ||
[[File:jmapB20100403.png|500px]] | [[File:jmapB20100403.png|500px]] | ||
| + | |||
| + | <br /> | ||
| + | |||
| + | 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:20100403stack.png]] <br> | ||
| + | |||
| + | Fitting parameters in GCS Model: Carrington Longitude: 260.785 degrees, Latitude: -26.273 degrees, Tilt Angle: 14.535 degrees, Aspect Ratio: .378943, Half Angular Width: 24.9751 <br> | ||
==GOES X-RAY FLUX== | ==GOES X-RAY FLUX== | ||
| − | GOES | + | [[File:20100403_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= | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403cor2A.avi COR2A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403cor2B.avi COR2B] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi1A.avi HI1A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi1B.avi HI1B] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi2A.avi HI2A] <br> | ||
| + | [http://solar.gmu.edu/wiki/upload/phess4/20100403hi2B.avi HI2B] <br> | ||
| + | |||
| + | =References= | ||
| + | *Brian Wood paper 2010 (density shell model with different orientations) | ||
| + | *Liu et al. 2011 ApJ (SEPs) | ||
| + | *Rouillard et al. 2011 ApJ (shock, SEPs) | ||
| + | *Moestl et al. 2010 GRL (HI modeling and ICME) | ||
| + | *Rollett et al. 2012 Sol. Phys. (kinematics) | ||
Latest revision as of 15:11, 5 August 2013
The April 05, 2010 CME erupted from Sun around 09:00 UT on April 03, associated with a flare from NOAA Active Region 11059 (S25 W03). The first signature as seen in ACE is of a shock front at 08:00 UT and a flux rope is observed by ACE at 11:30 UT.
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-Apr-03 Event
- paper http://arxiv.org/abs/1110.0827
- A well-behaved CME-ICME event (Jie)
- unsolved question:
explain the magnetic field profile of the ICME; how well do predictions perform?
Image Data
In-Situ Data
A combination of SWEPAM and MAG data from the ACE Satellite:
The blue lines are an approximation of the CME cloud and the red line denotes the shock.
Heliospheric Imaging
Jmaps from STEREO A and B along the CME leading edge position angle
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: 260.785 degrees, Latitude: -26.273 degrees, Tilt Angle: 14.535 degrees, Aspect Ratio: .378943, Half Angular Width: 24.9751
GOES X-RAY FLUX
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
References
- Brian Wood paper 2010 (density shell model with different orientations)
- Liu et al. 2011 ApJ (SEPs)
- Rouillard et al. 2011 ApJ (shock, SEPs)
- Moestl et al. 2010 GRL (HI modeling and ICME)
- Rollett et al. 2012 Sol. Phys. (kinematics)
