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published by the NASA/Goddard Space Flight Center
This video-based tutorial from the Goddard Space Flight Center provides lay explanations of the differences between solar flares and coronal mass ejections (CMEs). The strongest solar flares are almost always correlated with CME's. Both involve gigantic explosions of energy, but they emit different things, they travel differently, and have different effects on planets in our solar system. Solar flares look like sudden bursts of light, they contain tremendous energy, and travel at the speed of light. CMEs are plasma clouds containing enormous amounts of magnetized particles. CMEs travel over a million miles an hour, but well below the speed of light. Large CMEs can interrupt or overload electrical grids, create auroras, and degrade radio transmission. Both are widely studied by NASA missions such as Magnetospheric Multiscale (MMR) the Solar and Heliospheric Observatory (SOHO), and the Solar Dynamics Observatory (SDO).

NGSS Standards (4)

Subjects Levels Resource Types
Astronomy
- The Sun
= Magnetic Activity
= Space Weather
Electricity & Magnetism
- Electromagnetic Radiation
= Electromagnetic Spectrum
- Magnetic Fields and Forces
= Magnetic Fields
Modern Physics
- Plasma Physics
- High School
- Lower Undergraduate
- Informal Education
- Instructional Material
= Tutorial
- Audio/Visual
= Movie/Animation
Appropriate Courses Categories Ratings
- Physical Science
- Physics First
- Conceptual Physics
- Algebra-based Physics
- AP Physics
- Activity
- New teachers
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