2023-05-16T17:48:00-CME-001

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O:8:”stdClass”:10:{s:2:”id”;s:27:”2023-05-16T17:48:00-CME-001″;s:7:”catalog”;s:11:”M2M_CATALOG”;s:5:”start”;s:17:”2023-05-16T17:48Z”;s:6:”source”;s:0:””;s:6:”region”;N;s:4:”link”;s:59:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CME/25174/-1″;s:4:”note”;s:222:”Partial halo CME seen to the west-northwest in all coronagraph imagery in association with a fast loop which is seen erupting in SDO 193/171 off the western limb and flickering of magnetic field lines seen best in SDO 193.”;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:2:{i:0;a:11:{s:8:”time21_5″;s:17:”2023-05-16T19:59Z”;s:8:”latitude”;d:13;s:9:”longitude”;d:140;s:9:”halfAngle”;d:44;s:5:”speed”;d:1480;s:4:”type”;s:1:”O”;s:14:”isMostAccurate”;b:1;s:4:”note”;s:88:”More updated leading edge measurement using SOHO C2, SOHO C3, and STEREO A COR2 imagery.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/25176/-1″;s:9:”enlilList”;a:1:{i:0;a:13:{s:19:”modelCompletionTime”;s:17:”2023-05-16T19:32Z”;s:2:”au”;d:2;s:25:”estimatedShockArrivalTime”;N;s:17:”estimatedDuration”;N;s:7:”rmin_re”;N;s:5:”kp_18″;N;s:5:”kp_90″;N;s:6:”kp_135″;N;s:6:”kp_180″;N;s:9:”isEarthGB”;b:0;s:4:”link”;s:65:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/WSA-ENLIL/25178/-1″;s:10:”impactList”;a:2:{i:0;a:3:{s:14:”isGlancingBlow”;b:0;s:8:”location”;s:18:”Parker Solar Probe”;s:11:”arrivalTime”;s:17:”2023-05-18T00:04Z”;}i:1;a:3:{s:14:”isGlancingBlow”;b:0;s:8:”location”;s:13:”Solar Orbiter”;s:11:”arrivalTime”;s:17:”2023-05-17T19:53Z”;}}s:6:”cmeIDs”;a:1:{i:0;s:27:”2023-05-16T17:48:00-CME-001″;}}}}i:1;a:11:{s:8:”time21_5″;s:17:”2023-05-16T19:28Z”;s:8:”latitude”;d:13;s:9:”longitude”;d:153;s:9:”halfAngle”;d:39;s:5:”speed”;d:1795;s:4:”type”;s:1:”O”;s:14:”isMostAccurate”;b:0;s:4:”note”;s:149:”Preliminary measurement using early frames close to the occulting disk of SOHO and STEREO A. The speed is likely to decrease with additional imagery.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/25175/-1″;s:9:”enlilList”;N;}}s:13:”linked_events”;N;}