Space Weather
This movie takes us on a space weather journey from the center of the sun to solar eruptions in the sun's atmosphere all the way to the effects of that activity near Earth. The view starts in the core of the sun where atoms fuse together to create light and energy. Next we travel toward the sun's surface, watching loops of magnetic fields rise up to break through the sun's atmosphere, the corona. In the corona is where we witness giant bursts of radiation and energy known as solar flares, as well as gigantic eruptions of solar material called coronal mass ejections or CMEs. The movie follows one of these CME's toward Earth where it impacts and compresses Earth's own protective magnetic bubble, the magnetosphere. As energy and particles from the sun funnel along magnetic field lines near Earth, they ultimately produce aurora at Earth's poles.
Space Weather animation
Fusion
Ignition
Core
Loops
Breaching the surface of the Sun
Loops on the Sun's surface
Flares on the Sun
Prominence on the Sun
CME on the Sun
CME leaving the Sun
CME approaching Earth
Earth and magnetosphere revealed and CME Impact
Frontside reconnection and aurora
Backside reconnection and aurora
Aurora at the South pole
Credits
Please give credit for this item to:
Conceptual Image Lab, NASA/Goddard Space Flight Center
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Animators
- Walt Feimer (HTSI)
- Michael Lentz (USRA)
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Producer
- Walt Feimer (HTSI)
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Scientist
- Holly Gilbert (NASA/GSFC)
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Writer
- Karen Fox (ADNET Systems, Inc.)
Release date
This page was originally published on Thursday, September 20, 2012.
This page was last updated on Tuesday, December 17, 2024 at 12:16 AM EST.