2023-03-16T21:12:00-CME-001

Home

O:8:”stdClass”:10:{s:2:”id”;s:27:”2023-03-16T21:12:00-CME-001″;s:7:”catalog”;s:11:”M2M_CATALOG”;s:5:”start”;s:17:”2023-03-16T21:12Z”;s:6:”source”;s:6:”S30W35″;s:6:”region”;N;s:4:”link”;s:59:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CME/24277/-1″;s:4:”note”;s:389:”Faint CME seen in the SW of SOHO LASCO C2/C3 and STEREO A COR2. Limited STEREO A COR2 imagery available due to ongoing science campaign. The source is a filament eruption centered around S30W35 best seen in SDO AIA 304 starting around 2023-03-16T20:00Z. The eruption is also characterized by dimming in SDO AIA 193. The eruption is also seen in the the SW of STEREO A EUVI 195/304 imagery.”;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:”2023-03-17T02:37Z”;s:8:”latitude”;d:-51;s:9:”longitude”;d:35;s:9:”halfAngle”;d:31;s:5:”speed”;d:606;s:4:”type”;s:1:”C”;s:14:”isMostAccurate”;b:1;s:4:”note”;s:228:”No STEREO A COR2 imagery was used due to lack of available difference imagery. This measurement is based on the source location of the filament eruption and parameters were confirmed using a preliminary measurement in StereoCAT.”;s:11:”levelOfData”;i:0;s:4:”link”;s:67:”https://webtools.ccmc.gsfc.nasa.gov/DONKI/view/CMEAnalysis/24278/-1″;s:9:”enlilList”;N;}}s:13:”linked_events”;N;}