Building a 3-D Coronal Mass Ejection from 2-D Data
Using differences in polarization of light directly from the Sun vs. scattered from the CME electrons, it is possible to derive a distance of matter along the line-of-sight. This version is an enhanced version of animation ID 2950 with a color table enhanced to show fainter regions of the CME.
Movie viewing the CME reconstruction from different angles.
View of the CME towards the Earth
View of the CME from the side.
View of the CME from above.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
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Animator
- Tom Bridgman (Global Science and Technology, Inc.)
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Scientist
- Thomas Moran (CUA)
Missions
This page is related to the following missions:Series
This page can be found in the following series:Related papers
Moran, T.G. and Davila, J.M., 2004, Science 305, pp. 66-70.
Moran, T.G. and Davila, J.M., 2004, Science 305, pp. 66-70.
Datasets used
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SOHO/MDI [SOHO: Michelson Doppler Interferometer (MDI)]
ID: 96This dataset can be found at: http://sohowww.nascom.nasa.gov
See all pages that use this dataset -
LASCO/C2 (C2) [SOHO: Large Angle Spectrometric COronagraph (LASCO)]
ID: 160This dataset can be found at: http://sohowww.nascom.nasa.gov
See all pages that use this dataset
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.
Release date
This page was originally published on Thursday, July 1, 2004.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.