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STEREO Paris Conference

Gary, G. A. PowerPoint Presentation "On Determining the 3D Morphology and Plasma Properties of the Solar Corona"

Associated Movies:

November 6, 1996 CME

November 5-6, 1997 CME

Filament Eruption From TRACE

Computer Overload

3D CME Structure Movie 1

3D CME Structure Movie 2

3D CME Structure Movie 3

CME Simulation

CME Reconstruction Simulation (RADON)

Synthesized Active Region Rotation

Also see:

Gary, G. A., 1996, "Potential Field Extrapolation Using Three Components of Solar Vector Magnetogram with a Finite Field of View", Solar Phys., 163, 43.

Gary, G. A., 1997,  "Rendering Three-Dimensional Solar Coronal Structures"Solar Phys., 174, 241.

Gary, G. A., Davis, J. M., and Moore, R, 1998, ``On Analysis of Dual Spacecraft Stereoscopic Observations to Determine the Three-Dimensional Morphology and Plasma Properties of Solar Coronal Flux Tubes'', Solar Phys., 183, 45.

Gary, G. A., and Alexander, D., 1999, ``Constructing the Coronal Magnetic Field by Correlating Parameterized Magnetic Field Lines With Observed Coronal Plasma Structures'', Solar Phys., 186, 123.


 

Author: David H. Hathaway, david.hathaway@msfc.nasa.gov, (256) 544-7610
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812

 

Responsible Official: John M. Davis, john.m.davis@msfc.nasa.gov, (256) 544-7600
Mail Code SD50, NASA/Marshall Space Flight Center, Huntsville, AL 35812

 

Last revised 2002 March 14 - D. H. Hathaway