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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-06-29T09:00Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
STEREO A: SECCHI/COR2
Activity ID: 2026-06-29T09:00:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
Note: CME visible to the east in GOES CCOR-1 and faintly to the west in STEREO A COR2 imagery. The CME is not seen in real-time in SOHO LASCO C2/C3 due to a downlink data gap. The source is likely farsided as seen as moving field lines in SDO AIA 171 in ISWA and SDO AIA 193 starting around 2026-06-29T06:57Z. An estimated M4.0 class solar flare was observed on the farside from the point of view of the Solar Orbiter/STIX, located around longitude -158, at 2026-06-29T07:29Z.
Version 1 submitted on 2026-06-29T12:21Z by Mary Aronne
	
A Notification with ID 20260629-AL-001 was sent on 2026-06-29T13:30Z

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 -144.0 -8.0 631.0 C 18.0 2026-06-29T13:11Z Measurement based on the best fit between GOES CCOR-1 and STEREO A COR2 imagery in SWPC_CAT. The leading edge is faint and unclear in running difference imagery, and this measurement is approximate. 1: Result 1 (2.0 AU)
Solar Orbiter = 2026-07-01T18:11Z
Mary Aronne on 2026-06-29T12:22Z



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