+ Visit NASA.gov + Advanced Search   + About the Server   + Animation List   + How to Use the Server   + RSS Feeds Previous Animation Next Animation 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. Duration: 4.0 seconds Available formats:   640x480 (30 fps) Frames   640x480 (30 fps) MPEG-1   2 MB   320x240 (30 fps) MPEG-1   568 KB   320x240     JPEG         6 KB   320x240     JPEG         6 KB   1280x720 (30 fps) MPEG-2   8 MB   1280x720 (30 fps) Frames How to play our movies    View of the CME towards the Earth Available formats:   2560 x 1920     TIFF 1 MB   320 x 240         JPEG 5 KB    View of the CME from the side. Available formats:   2560 x 1920     TIFF 1 MB   160 x 80           PNG   8 KB   320 x 240         JPEG 7 KB   80 x 40             PNG   2 KB    View of the CME from above. Available formats:   2560 x 1920     TIFF 1 MB   320 x 240         JPEG 6 KB Animation Number: 2958 Animator: Tom Bridgman (SVS) (Lead) Completed: 2004-07-01 Scientist: Thomas Moran (CUA) Instruments: SOHO/MDI   SOHO/LASCO/C2 Data Collected: 1999-06-29 Series: 3-D Coronal Mass Ejections Keywords: SVS >> CME SVS >> Coronal Mass Ejection SVS >> HDTV DLESE >> Space science SVS >> Sun Science paper: Moran, T.G. and Davila, J.M., 2004, Science 305, pp. 66-70.     Please give credit for this item to NASA/Goddard Space Flight Center Scientific Visualization Studio Back to Top + Privacy Policy and Important Notices + Reproduction Guidelines NASA Official: SVS Contact: Curator: