Bastille Day Flare Without Matter Motion
Fly-in of TRACE full sun image to the flare location. Fade to a model of the field lines with a magnetogram of the solar surface. Pull back out to display a movie of flare images. This version does not show the matter motion along the field lines.
Zoom in to the Bastille Day flare (1998) and fade to a model of the magnetic field lines in the region.

Video slate image reads, "TRACE
'Bastille Day' Flare
Magnetic Field Model".
Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
-
Animators
- Tom Bridgman (Global Science and Technology, Inc.)
- Greg Shirah (NASA/GSFC)
-
Scientist
- G. Aulanier (Naval Research Laboratory)
Missions
This page is related to the following missions:Series
This page can be found in the following series:Related papers
Aulanier, G., DeLuca, E.E., Antiochos, S.K., McMullen, R.A., & Golub, L. 2000, Astrophysical Journal, 540, 1126
Aulanier, G., DeLuca, E.E., Antiochos, S.K., McMullen, R.A., & Golub, L. 2000, Astrophysical Journal, 540, 1126
Datasets used
-
[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 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, June 13, 2000.
This page was last updated on Wednesday, May 3, 2023 at 1:58 PM EDT.