Massive Solar Eruption Close-up
SDO observed the flare's peak at 1:41 AM ET. SDO recorded these images in extreme ultraviolet light that show a very large eruption of cool gas. It is somewhat unique because at many places in the eruption there seems to be even cooler material — at temperatures less than 80,000 K.
This video uses the full-resolution 4096 x 4096 pixel images at a one minute time cadence to provide the highest quality, finest detail version possible.
It is interesting to compare the event in different wavelengths because they each see different temperatures of plasma. See the transcript for more notes on this.
Frames for each wavelength are available on these separate pages: 304, 171, 211, and1700.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Animator
- Tom Bridgman (GST)
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 AIA 1700 (A.K.A. 1700 Filter) (Collected with the AIA sensor)
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setSDO AIA 171 (A.K.A. 171 Filter) (Collected with the AIA sensor)
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setSDO AIA 211 (A.K.A. 211 Filter) (Collected with the AIA sensor)
Dataset can be found at: http://jsoc.stanford.edu/
See more visualizations using this data setSDO AIA 304 (A.K.A. 304 Filter) (Collected with the AIA sensor)
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.