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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-24T12:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-05-24T12:12:00-CME-001 (version 2)
Source Location: N45W75
Note Keyword:
3P: 3-part structure CME
GAP: Data gap
Source Signature Keyword:
PEA: Post eruption arcade
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: This CME is visible to the northwest in SOHO LASCO C2/C3 imagery. The source is likely an eruption centered near N45W75 starting around 2024-05-24T11:25Z as seen in SDO AIA 131, 171, 193, 304 imagery, but the center of the eruption could be closer to the limb/on limb. A strong opening of field lines is visible in SDO AIA 171 and 193 imagery, with post eruptive arcades starting to form around 12:00Z.
Submitted on 2024-05-25T19:06Z by Anna
Chulaki
No Notification has been sent for this activity yet.
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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
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
97.0 |
58.0 |
518.0 |
C |
39.0 |
2024-05-24T19:09Z |
Analysis based on fit with two coronagraphs, indicating that the source longitude is higher than estimated (behind the limb). |
Not modeled
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Anna Chulaki on 2024-05-25T19:06Z |
CME Analysis
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M2M_CATALOG |
LE
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false |
SWPC_CAT |
75.0 |
63.0 |
529.0 |
C |
42.0 |
2024-05-24T19:11Z |
Measured longitude based on the source location. Due to a data gap in STEREO A during this time, there is no stereoscopic viewpoint available to confirm the measurement. The measured parameters may very slightly as a result. |
Not modeled
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Mattie Anastopulos on 2024-05-24T17:11Z |
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