Comparison: Solar Maximum from SOHO/EIT
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- Visualizations by:
- Steele Hill
- View full credits
A short movie of the Sun at maximum solar activity as seen in ultraviolet light. These images are collected in ultraviolet light (a wavelength of 195Å or 19.5 nanometers) which is only visible to space-based instruments. In visible light, the bright white regions in these images would probably correspond to sunspots.
At solar maximum, we see many bright active regions which tend to form in bands in the northern and southern hemispheres. Many of the active regions may eventually launch solar flares or coronal mass ejections (CME).
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio
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Animators
- Steele Hill (Wyle Information Systems) [Lead]
- Tom Bridgman (GST)
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Producer
- Rani Gran (NASA/GSFC)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Datasets used in this visualization
SOHO SOHO/EIT 195 (A.K.A. 195 Filter) (Collected with the Extreme-UV Imaging Telescope (EIT) sensor)
NASA and ESA
2002-08-18T00:00 - 2002-08-19T00:00
Dataset can be found at: http://sohowww.nascom.nasa.gov
See more visualizations using this data setNote: While we identify the data sets used in these visualizations, we do not store any further details, nor the data sets themselves on our site.
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