Sun  ID: 4178

As Seen by STEREO-B: The Carrington-Class CME of 2012

Like SDO, STEREO-B did not have a direct view of the coronal mass ejection (CME) launched by the sun on July 23, 2012. However, the active region involved was very close to the limb of the sun (lower left quadrant) and STEREO-B provided an excellent view of plasma launched in both ultraviolet light and the white-light coronagraph.
 

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Visualization Credits

Tom Bridgman (GST): Lead Animator
Scott Wiessinger (USRA): Producer
Joe Gurman (NASA/GSFC): Scientist
Laurence Schuler (ADNET Systems Inc.): Project Support
Ian Jones (ADNET Systems Inc.): Project Support
Please give credit for this item to:
NASA's Scientific Visualization Studio

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Missions:
SDO
STEREO

Data Used:
STEREO-B/Extreme UltraViolet Imager/195 Angstroms 2012-07-23T00:00:00 - 2012-07-23T23:59:59
STEREO-B/Extreme UltraViolet Imager/304 Angstroms 2012-07-23T00:00:00 - 2012-07-23T23:59:59
STEREO-B/Coronograph 2 2012-07-23T00:00:00 - 2012-07-23T23:59:59
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:
The Carrington-Class CME of 2012

Keywords:
SVS >> HDTV
SVS >> Solar Wind
SVS >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Flares
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Solar Ultraviolet
SVS >> Space Weather
SVS >> Hyperwall
SVS >> SDO
SVS >> Heliophysics
SVS >> STEREO
SVS >> Corona
NASA Science >> Sun
GCMD >> Earth Science >> Sun-earth Interactions >> Solar Activity >> Coronal Mass Ejections

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

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