2023-04-06T03:24:00-CME-001

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O:8:”stdClass”:10:{s:2:”id”;s:27:”2023-04-06T03:24:00-CME-001″;s:7:”catalog”;s:11:”M2M_CATALOG”;s:5:”start”;s:17:”2023-04-06T03:24Z”;s:6:”source”;s:0:””;s:6:”region”;N;s:4:”link”;s:59:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CME/24520/-1″;s:4:”note”;s:266:”This CME is visible to the SE in SOHO LASCO C2/C3 coronagraph. Data gap in STEREO A COR2 coronagraph for the entire CME. The source is likely an eruption on the far side of the Sun, behind the SE limb, seen as opening field lines in SDO AIA 171 at 2023-04-06T02:36Z.”;s:11:”instruments”;a:2:{i:0;a:1:{s:11:”displayName”;s:14:”SOHO: LASCO/C2″;}i:1;a:1:{s:11:”displayName”;s:14:”SOHO: LASCO/C3″;}}s:8:”analyses”;a:1:{i:0;a:11:{s:8:”time21_5″;s:17:”2023-04-06T09:43Z”;s:8:”latitude”;d:-11;s:9:”longitude”;d:-151;s:9:”halfAngle”;d:28;s:5:”speed”;d:507;s:4:”type”;s:1:”C”;s:14:”isMostAccurate”;b:1;s:4:”note”;s:428:”Measured using only SOHO LASCO C2 and C3 difference imagery, due to data gap in STEREO A COR2. Some uncertainty in this measurement comes from assuming this longitude to be the same as the measured longitude of a preceding CME where both SOHO LASCO C2/C3 and STEREO A COR2 were available. This CME was one of many seen in rapid succession moving in the same direction and with similar moving field line signatures in UV imagery.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/24521/-1″;s:9:”enlilList”;N;}}s:13:”linked_events”;N;}