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CME Analysis Information (for CME activity ID: 2024-03-09T22:36:00-CME-001)
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
Image Type: running difference
Speed (km/s): 841.0
Speed measured at height (Rs): None Entered
Type: C
Direction (LON/LAT in HEEQ): -126.0/ 23.0
Half Angular Width (degree): 52.0
Minor Half-width (degree): None Entered
Tilt (degree): None Entered
Time@21.5: 2024-03-10T02:51Z
Info/Session URL: None Entered
Note: 
A very approximate analysis of the brighter bulk of this CME (vs fainter likely more backsided shock). Analysis is based on the fitting of the front with one coronagraph (SOHO) in swpc_cat tool. The uncertainty of the CME longitude is significant because the source is behind the limb based on the lower coronal signatures) and the CME is not seen in STEREO coronagraph because of a large data gap. The longitude can vary from -110 to -150 degrees, so the speed of the CME could be even faster. Helioseismology data from GONG indicate that the former AR 3590 was at ~-177 degrees at the time and so is unlikely to be the source of this CME.
Measurement Feature Code(s):
LE: Leading Edge
General Keyword(s):
Submitted on 2024-03-10T18:02Z by Anna Chulaki

A Notification with ID 20240310-AL-003 was sent on 2024-03-10T17:33Z

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 2024-03-10T17:10Z 2.0
No or little impact to Earth. Parker Solar Probe = 2024-03-11T17:00Z
WSA-ENLIL+Cone 2024-03-10T17:24Z 5.5
No or little impact to Earth. Juno = 2024-03-24T18:00Z

All directly linked activities:
2024-03-09T22:36:00-CME-001


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