Incandescent Sun
- Visualizations by:
- Tom Bridgman
- View full credits
This video takes SDO images and applies additional processing to enhance the structures visible. While there is no scientific value to this processing, it does result in a beautiful, new way of looking at the sun. The original frames are in the 171 angstrom wavelength of extreme ultraviolet. This wavelength shows plasma in the solar atmosphere, called the corona, that is around 600,000 Kelvin. The loops represent plasma held in place by magnetic fields. They are concentrated in "active regions" where the magnetic fields are the strongest. These active regions usually appear in visible light as sunspots. The events in this video represent 24 hours of activity on September 25, 2011.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Animators
- Tom Bridgman (GST) [Lead]
- Scott Wiessinger (KBRwyle)
Video editor
- Scott Wiessinger (KBRwyle)
Producer
- Scott Wiessinger (KBRwyle)
Missions
This visualization is related to the following missions:Series
This visualization can be found in the following series:Tapes
This visualization originally appeared on the following tapes:- None
Datasets used in this visualization
SDO
Dataset can be found at: http://sdo.gsfc.nasa.gov/
See more visualizations using this data setSDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER
Dataset can be found at: http://jsoc.stanford.edu/
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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