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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-04-17T22:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-04-17T22:24:00-CME-001 (version 1)
Note Keyword:
Faint: Faint event; may affect type assignment
GAP: Data gap
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
L: Loop
Note: Fast, thin CME seen to the E in SOHO LASCO C2/C3. The source for this CME is uncertain, observed as some field line movement outside of the E limb starting around 2024-04-17T21:00Z in SDO AIA 171. This could correspond to some activity near AR 3645 observed in SDO AIA 171/193 that "bubbles" low at that same timestamp before a more reactive eruption starting 2024-04-17T21:55Z. However, low confidence during the CME measurement process (would be a thinner than 10 degree half-width, and no STEREO COR2A data to triangulate with) from this longitude casts some doubt on this.

Submitted on 2024-04-18T18:03Z 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, 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 Plane-of-sky NONE -5.0 592.0 C 10.0 2024-04-18T04:38Z Plane-of-sky measurement using only SOHO LASCO C2/C3 due to low source confidence and lack of STEREO COR2A imagery to triangulate with due a data gap. The source could be AR 3465 around S10E25 based on EUV imagery, but this produces a <10 half-width fit. Not modeled Tony Iampietro on 2024-04-18T18:06Z



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