2023-04-23T12:48:00-CME-001

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O:8:”stdClass”:10:{s:2:”id”;s:27:”2023-04-23T12:48:00-CME-001″;s:7:”catalog”;s:11:”M2M_CATALOG”;s:5:”start”;s:17:”2023-04-23T12:48Z”;s:6:”source”;s:0:””;s:6:”region”;N;s:4:”link”;s:59:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CME/24751/-1″;s:4:”note”;s:220:”This CME is visible to the NW in SOHO LASCO C2/C3 and STEREO A COR2 imagery. The source is likely the faint field line movement visible beyond the NW limb in SDO AIA 171 and 193 imagery starting around 2023-04-23T10:30Z.”;s:11:”instruments”;a:3:{i:0;a:1:{s:11:”displayName”;s:14:”SOHO: LASCO/C2″;}i:1;a:1:{s:11:”displayName”;s:14:”SOHO: LASCO/C3″;}i:2;a:1:{s:11:”displayName”;s:21:”STEREO A: SECCHI/COR2″;}}s:8:”analyses”;a:1:{i:0;a:11:{s:8:”time21_5″;s:17:”2023-04-23T21:15Z”;s:8:”latitude”;d:43;s:9:”longitude”;d:104;s:9:”halfAngle”;d:10;s:5:”speed”;d:427;s:4:”type”;s:1:”S”;s:14:”isMostAccurate”;b:1;s:4:”note”;s:151:”Measurement based on the best fit between SOHO LASCO C2 and STEREO A COR2. The leading edge is very diffuse and difficult to track after early imagery.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/24752/-1″;s:9:”enlilList”;N;}}s:13:”linked_events”;N;}