Solar Tsunamis - View with a Spin
Push-in to a region of the Sun to witness a 'solar tsunami' after a flare event. The tsunami moves hot gas (bright) out of the region, revealing cooler regions (darker) below. This view rotates on the push-in to keep the region of the flare event visible (to the left in the final frame).
Closeup view of the tsunami (with rotation)
A view of the Sun before the event.
Close-up TRACE field-of-view as the wave moves across the image.
The wave has passed, and the region behind it is darker.
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
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Animator
- Tom Bridgman (Global Science and Technology, Inc.)
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Scientists
- Craig DeForest (SwRI)
- Meredith Wills-Davey (SwRI)
Series
This page can be found in the following series:Datasets used
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SOHO/EIT [SOHO: Extreme-UV Imaging Telescope (EIT)]
ID: 94This dataset can be found at: http://sohowww.nascom.nasa.gov
See all pages that use this dataset -
[TRACE]
ID: 106The TRACE satellite views the Sun at ultraviolet wavelengths with high temporal (approximately 1-12 seconds) and spatial (1 arcsecond per pixel) resolution. Launched on April 2, 1998, it orbits the Earth in a Sun-synchronous orbit.
This dataset can be found at: http://sunland.gsfc.nasa.gov/smex/trace/
See all pages that use this dataset -
Continuum [SOHO: Michelson Doppler Interferometer (MDI)]
ID: 619This dataset can be found at: http://sohowww.nascom.nasa.gov
See all pages that use this dataset
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.
Release date
This page was originally published on Tuesday, March 8, 2005.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.