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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Datasets used in this visualization
STEREO-B EUVI (195 Angstroms)ID: 832Observed Data Collected with Extreme UltraViolet Imager 2012-07-23T00:00:00 - 2012-07-23T23:59:59
STEREO-B EUVI (304 Angstroms)ID: 833Observed Data Collected with Extreme UltraViolet Imager 2012-07-23T00:00:00 - 2012-07-23T23:59:59
STEREO-B COR2ID: 834Observed Data Collected with Coronograph 2 2012-07-23T00:00:00 - 2012-07-23T23:59:59
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