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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-11-04T17:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-11-04T17:24:00-CME-001 (version 1)
Source Location: S07E38
Active Region Number: 13883
Note Keyword:
DFL: Likely deflection of the event within the FOV
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
DIM: Dimming
Morphology Keyword:
O: Other
Note: CME seen to the E in all coronagraphs, with minimal frames in STEREO COR2A due to a data gap. This CME front is comprised of a slower northern piece and a faster southern piece which still relatively travel together, causing a distortion in the front as it travels from earliest frames -> later frames. The source is the double peaked M3.7 and M5.5 flare from AR 3883 (S07E38), which began at 2024-11-04T15:26Z in SDO AIA 131 with additional field line movement and very slight dimming observed in SDO AIA 171/193/211.
Submitted on 2024-11-05T01:53Z by Tony
Iampietro
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 |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-47.0 |
4.0 |
388.0 |
S |
28.0 |
2024-11-05T02:08Z |
Triangulated measurement using STEREO C2/C3 and STEREO COR2A, with notable difficulty using COR2A running difference imagery with only two available frames over the duration of this CME due to a data gap. The on-disk source flares observed in SDO AIA 131 also assisted in triangulating this event to this source, ruling out far-sided fits. |
1: Result 1 (2.0 AU)
Earth = 2024-11-08T10:00Z
(PE: 19.5 h)
Lucy = 2024-11-07T14:00Z
Parker Solar Probe = 2024-11-07T10:00Z
Solar Orbiter = 2024-11-07T10:00Z
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Tony Iampietro on 2024-11-05T01:55Z |
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