Model for Coronal Mass Ejections
A coronal mass ejection (CME) is a massive burst of solar wind, other light isotope plasma, and magnetic fields rising above the solar corona or being released into space.
A coronal mass ejection (CME) is a massive burst of solar wind, other light isotope plasma, and magnetic fields rising above the solar corona or being released into space.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Conceptual Image Lab
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Animator
- Walt Feimer (HTSI)
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Scientist
- Therese Kucera (NASA/GSFC)
Release date
This page was originally published on Wednesday, April 27, 2005.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.