Sun  ID: 2509

A Multi-Mission View of the AR9906 Solar Flare with Instrument Labels

Here's a view of the Sun, from the point of view of a fleet of Sun-observing spacecraft - SOHO, TRACE, and RHESSI. The time scales of the data samples in this visualization range from six hours to as short as 12 seconds and the display rate varies throughout the movie. The region and event of interest is the solar flare over solar active region AR9906 on April 21, 2002. In this visualization, the instrument names appear in a color roughly matching the color used for the data, and black corresponds to no (current) instrument coverage.

Visualization Credits

Tom Bridgman (Global Science and Technology, Inc.): Lead Animator
Please give credit for this item to:
NASA/Goddard Space Flight Center Scientific Visualization Studio. A special thanks to all those who contributed data and advice without which this product would not have been possible (in no particular order): Alexander Kosovichev (Stanford University), Todd Hoeksema (Stanford University), Steele Hill (L-3 Communications Analytics Corporation/GSFC), Brian R. Dennis (NASA/GSFC), Peter T. Gallagher (L-3 Communications Analytics Corporation/GSFC), Joseph B. Gurman (NASA/GSFC), Nathan Rich (Interferometrics Inc./NRL), Bernhard Fleck (NASA/GSFC), Craig DeForest (SwRI), Philip Scherrer (Stanford University)

Short URL to share this page:
https://svs.gsfc.nasa.gov/2509

Missions:
RHESSI
SOHO
TRACE

Data Used:
TRACE/Optical Telescope/195 Angstroms
2002/04/21T00:10:59-2002/04/21T07:58:34
RHESSI/X-ray Imaging Spectrometer
2002/04/21T00:42:52-2002/04/21T01:32:18
The RHESSI instrument is an imaging spectrometer observing the Sun at X-ray to gamma-rays (photon energies of 3 keV to 17 MeV) at time resolutions of a few seconds. (eV stands for "electron volt" and is a unit of energy. Note that photons of visible light have energies of 2-3 eV. 1 keV is a thousand electron volts and 1 MeV is a million electron volts.
SOHO/Michelson Doppler Interferometer (MDI)/Continuum
NASA and ESA - 2002/04/10T23:59:31-2002/04/21T17:35:31
SOHO/Large Angle Spectrometric COronagraph (LASCO)/C2 also referred to as: LASCO/C2
NASA and ESA - 2002/04/18T00:06:05-2002/04/23T23:51:10
SOHO/Large Angle Spectrometric COronagraph (LASCO)/C3 also referred to as: LASCO/C3
NASA and ESA - 2002/04/18T00:18:05-2002/04/23T23:42:05
SOHO/Extreme-UV Imaging Telescope (EIT)/195 Filter also referred to as: SOHO/EIT 195
NASA and ESA - 2002/04/20T00:00:10-2002/04/21T23:52:09
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.

This item is part of this series:
Multi-Mission Solar Movie

Keywords:
SVS >> Active Region 9906
SVS >> HDTV
SVS >> SOHO
DLESE >> Space science
SVS >> X-ray
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Active Regions
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Flares
SVS >> Hyperwall
SVS >> RHESSI
SVS >> TRACE
NASA Science >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Coronal Mass Ejections
SVS >> Visible Light Imaging
SVS >> Extreme Ultraviolet Imaging
SVS >> EUV Imaging
SVS >> X-ray Imaging

GCMD keywords can be found on the Internet with the following citation: Olsen, L.M., G. Major, K. Shein, J. Scialdone, S. Ritz, T. Stevens, M. Morahan, A. Aleman, R. Vogel, S. Leicester, H. Weir, M. Meaux, S. Grebas, C.Solomon, M. Holland, T. Northcutt, R. A. Restrepo, R. Bilodeau, 2013. NASA/Global Change Master Directory (GCMD) Earth Science Keywords. Version 8.0.0.0.0