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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-06-17T11:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-06-17T11:24:00-CME-001 (version 1)
Note Keyword:
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
L: Loop
Note: Faint CME visible to the NW in SOHO LASCO C2/C3 and STEREO A COR2. The source is not visible on the disk in available EUV imagery, but there is possibly some field line movement visible between frames 10:35Z and 10:55Z in STEREO A EUVI 195 and 304 imagery at a fairly high northern latitude and beyond the W limb as seen from STEREO A.

Submitted on 2024-06-17T18:46Z by Mary Aronne

A Notification with ID 20240618-AL-001 was sent on 2024-06-18T14:35Z

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) Submitted By
CME Analysis M2M_CATALOG LE true SWPC_CAT 144.0 24.0 974.0 C 31.0 2024-06-17T14:36Z Measurement based on best fit between SOHO LASCO C2/C3 and STEREO A COR2 in SWPC_CAT. 1: Result 1 (2.0 AU)
Solar Orbiter = 2024-06-20T01:46Z
OSIRIS-APEX = 2024-06-19T22:00Z
2: Result 2 (5.5 AU)
Solar Orbiter = 2024-06-20T01:31Z
Juno = 2024-07-04T12:00Z
OSIRIS-APEX = 2024-06-19T22:00Z
Mary Aronne on 2024-06-17T18:46Z



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