TRACE Observes Flows over Active Regions (Fast Play)
Zoom in on the Sun to show the outflow region.
Full-disk view of the Sun with SOHO-EIT around the time of the TRACE observations.
Close-up view of the outflow region with TRACE.
Video slate image reads "TRACE Observes Flows over Active Regions (Fast play)".
For More Information
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
-
Animator
- Tom Bridgman (Global Science and Technology, Inc.)
-
Scientists
- Amy R. Winebarger (NRL)
- Edward E. DeLuca (CfA)
- Leon Golub (CfA)
Release date
This page was originally published on Wednesday, May 15, 2002.
This page was last updated on Wednesday, May 3, 2023 at 1:57 PM EDT.
Series
This visualization can be found in the following series:Papers used in this visualization
'Steady Flows Detected in Extreme-Ultraviolet Loops', Amy R. Winebarger, Harry Warren, Adriaan van Ballegooijen, Edward E. DeLuca,Leon Golub. The Astrophysical Journal, Volume 567, Issue 1, pp. L89-L92.
Datasets used in this visualization
-
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
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.