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CME Analysis Information (for CME activity ID: 2025-11-29T06:15:00-CME-001)
Measurement Creation Time:
Catalog: M2M_CATALOG
Data Level: 0 (0=real-time, 1=real-time and checked by supervising forecaster, 2=retrospective science level data analysis)
Use as primary measurement: true
Measurement Technique: SWPC_CAT

Detecting Instruments:

SOHO: LASCO/C2

SOHO: LASCO/C3

STEREO A: SECCHI/COR2

GOES: CCOR-1

Image Type: running difference
Speed (km/s): 868.0
Speed measured at height (Rs): None Entered
Type: C
Direction (LON/LAT in HEEQ): -86.0/ 0.0
Half Angular Width (degree): 23.0
Minor Half-width (degree): None Entered
Tilt (degree): None Entered
Time@21.5: 2025-11-29T10:12Z
Info/Session URL: None Entered
Note:

Analysis based on the fit with all three coronagraphs (SOHO LASCO C2/C3, STEREO A COR2 and GOES CCOR-1). The source is likely the southern lobe of what looks like a three-pronged prominence eruption from/behind the NE limb, seen starting at 2025-11-29T05:36Z in GOES SUVI 304.

Measurement Feature Code(s):

LE: Leading Edge

General Keyword(s):

Version 1 submitted on 2025-11-29T21:43Z by Anna Chulaki
Version 2 submitted on 2025-11-29T21:45Z by Anna Chulaki

A Notification with ID 20251129-AL-004 was sent on 2025-11-29T23:28Z

The List of WSA-ENLIL Results:

Model Name	Model Completion Time	AU	CME Input(s)	Predicted Earth Impact	Predicted Other Location(s) Impact
WSA-ENLIL+Cone	2025-11-29T22:51Z	2.0		No or little impact to Earth.	Parker Solar Probe = 2025-11-30T02:10Z

All directly linked activities:

2025-11-29T06:15:00-CME-001

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