2023-04-26T11:00:00-CME-001

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O:8:”stdClass”:10:{s:2:”id”;s:27:”2023-04-26T11:00:00-CME-001″;s:7:”catalog”;s:11:”M2M_CATALOG”;s:5:”start”;s:17:”2023-04-26T11:00Z”;s:6:”source”;s:0:””;s:6:”region”;N;s:4:”link”;s:59:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CME/24804/-1″;s:4:”note”;s:275:”CME seen to the northeast following the path of 2023-04-26T07:00Z; no source is easily identified on the disk or on the limb, so the CME may be associated with far-side activity. There is high amount of uncertainty in the longitude of the CME, possibly as much as 40 degrees.”;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:”2023-04-26T18:27Z”;s:8:”latitude”;d:33;s:9:”longitude”;d:-99;s:9:”halfAngle”;d:35;s:5:”speed”;d:487;s:4:”type”;s:1:”S”;s:14:”isMostAccurate”;b:1;s:4:”note”;s:316:”Leading edge measurement. Triangulation using STEREO A is poor and provides a range of possible longitudes. No source is easily identified on the disk or on the limb, so the CME may be associated with far-side activity. There is high amount of uncertainty in the longitude of the CME, possibly as much as 40 degrees.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/24805/-1″;s:9:”enlilList”;a:1:{i:0;a:13:{s:19:”modelCompletionTime”;s:17:”2023-04-26T18:54Z”;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/24810/-1″;s:10:”impactList”;a:1:{i:0;a:3:{s:14:”isGlancingBlow”;b:0;s:8:”location”;s:4:”Mars”;s:11:”arrivalTime”;s:17:”2023-05-02T04:00Z”;}}s:6:”cmeIDs”;a:3:{i:0;s:27:”2023-04-26T11:00:00-CME-001″;i:1;s:27:”2023-04-26T11:12:00-CME-001″;i:2;s:27:”2023-04-26T14:36:00-CME-001″;}}}}}s:13:”linked_events”;N;}