Incandescent Sun

  • Released Wednesday, May 23, 2012
  • Updated Friday, October 9, 2015 at 1:20PM
  • ID: 10990

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.
Still of lower east limb CME in progress.

Still of lower east limb CME in progress.



Credits

Please give credit for this item to:
NASA/Goddard Space Flight Center


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 AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
JOINT SCIENCE OPERATIONS CENTER

Note: 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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