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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-25T16:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-07-25T16:00:00-CME-001 (version 1)
Source Location: S07W85
Active Region Number: 13751
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Ha: Bright emission (likely H-alpha emission)
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: CME seen to the W in SOHO only, due to an ongoing STEREO COR2A data gap covering this event. Source is an M1.3 class flare from AR 13751 which peaked at 2024-07-25T15:37Z, observed in SDO AIA 131. Also observed as opening field lines in SDO AIA 171/193/211 and filament material ejecting in SDO AIA 304 accompanying the flare.
Submitted on 2024-07-26T01:08Z by Tony Iampietro

No Notification has been sent for this activity yet.

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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME
 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 85.0 2.0 456.0 S 27.0 2024-07-25T23:56Z Measurement only using SOHO C2/C3 due to a STEREO COR2A data gap, but high confidence in the source of W85 based on SDO imagery and visual fit in swpc_cat. 1: Result 1 (2.0 AU)
Mars = 2024-07-30T11:00Z
OSIRIS-APEX = 2024-07-27T21:00Z
Tony Iampietro on 2024-07-26T01:09Z



All directly linked activities:
2024-07-25T15:27:00-FLR-001
FLR Type: M1.3


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