Stereo Captures Eruption and CME
On May 1, 2013, NASA's Solar Terrestrial Relations Observatory Ahead (STEREO-A) satellite along with its twin STEREO Behind (STEREO-B), observed an active region (right) of the sun erupt. This eruption, called a coronal mass ejection, or CME, sent plasma streaming out through the solar system. STEREO has an extreme ultraviolet camera similar to the Solar Dynamics Observatory (SDO) satellite, but it also has coronagraph telescopes like the European Space Agency/NASA Solar and Heliospheric Observatory (SOHO) where the bright sun is blocked by a disk so it does not overpower the fainter solar atmosphere. As a result, using its two inner coronagraphs, STEREO was able to track the CME from the solar surface out to 6.3 million miles.
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Please give credit for this item to:
NASA's Goddard Space Flight Center
MissionsThis visualization is related to the following missions:
Datasets used in this visualization
STEREO-AID: 186Collected with Coronograph 1 (COR1)
STEREO-AID: 187Collected with Coronograph 2 (COR2)
STEREO 304 AngstromsID: 624Collected with Extreme UltraViolet Imager (EUVI)
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.