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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-06-03T11:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2026-06-03T11:48:00-CME-001 (version 1)
Source Location: N14W16
Active Region Number: 14455
Note Keyword:
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
EUVW: EUV Wave
Morphology Keyword:
Note: This CME is visible as a partial halo to the north/northwest in SOHO LASCO C2/C3 and GOES CCOR-1 imagery, and to the northeast in STEREO A COR2 imagery. The source is an X1.0 flare and subsequent eruption from Active Region 14455 (N14W16) starting around 2026-06-03T11:20Z as seen in SDO AIA 131/171/193/304, GOES SUVI 131/171/195/284/304, and STEREO A EUVI 195/304 imagery. The associated ejecta displays a southeast deflection as seen in SDO AIA 304 imagery. A faint EUV wave is observed moving northwest of the eruption site, however, in SDO AIA 193 imagery.
Version 1 submitted on 2026-06-03T13:28Z by Mattie Anastopulos
	
A Notification with ID 20260603-AL-011 was sent on 2026-06-03T16:31Z
A Notification with ID 20260603-AL-013 was sent on 2026-06-03T18:26Z
A Notification with ID 20260603-AL-014 was sent on 2026-06-03T23:21Z

The List of CME Analysis already entered:
Event Type Catalog
Measurement TypeCME measurement type: Leading Edge (LE), Shock Front (SH), Right Hand Boundary (RHB), Left Hand Boundary (LHB), Black/White Boundary (BW), Prominence Core (COR), Disconnection Front (DIS), Trailing Edge (TE).
Prime?"primary flag" which is either True or False. If there are multiple CME analysis entries for a single CME, this flag would indicate which analysis is considered most accurate per measurement type. This is a helpful flag if you would like to download only one most accurate CME analysis per CME per Measurement Type
Technique Long Lat Speed Type Half Width Time 21.5 Note WSA-ENLIL+Cone Result(s) Measured On Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT 19.0 32.0 1433.0 O 37.0 2026-06-03T13:49Z A remeasurement of the two-lobed bulk front with more imagery. 1: Result 1 (2.0 AU)
Earth = 2026-06-05T07:45Z
Juice = 2026-06-06T20:31Z
OSIRIS-APEX = 2026-06-05T23:13Z
STEREO A = 2026-06-05T18:48Z
Europa Clipper = 2026-06-06T21:00Z
2: Result 2 (2.0 AU)
Earth = 2026-06-04T23:44Z
Juice = 2026-06-06T11:49Z
OSIRIS-APEX = 2026-06-05T14:55Z
STEREO A = 2026-06-05T13:58Z
Europa Clipper = 2026-06-06T12:00Z
Mattie Anastopulos on 2026-06-03T15:57Z
CME Analysis M2M_CATALOG SH true SWPC_CAT 12.0 16.0 1405.0 O 43.0 2026-06-03T13:57Z Approximate analysis of the faint partial halo shock front of this CME based on the fit with GOES CCOR-1 coronagraph, in which this front is seen clearer. LASCO imagery is also used. The front is not seen/clear in STEREO A COR2 coronagraph. 1: Result 1 (2.0 AU)
Earth = 2026-06-05T01:33Z
Europa Clipper = 2026-06-06T12:17Z
Juice = 2026-06-06T15:54Z
OSIRIS-APEX = 2026-06-05T16:09Z
STEREO A = 2026-06-05T15:06Z
Anna Chulaki on 2026-06-03T15:32Z
CME Analysis M2M_CATALOG LE false SWPC_CAT 20.0 30.0 905.0 C 41.0 2026-06-03T15:11Z Very preliminary, approximate analysis of the two-lobed bulk of the CME with very early imagery based on the fit in coronagraphs. Not modeled Anna Chulaki on 2026-06-03T13:46Z



All directly linked activities:
2026-06-03T11:19:00-FLR-001
FLR Type: X1.0


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