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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-01T23:09Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-10-01T23:09:00-CME-001 (version 3)
Source Location: S17E18
Active Region Number: 13842
Note Keyword:
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: Developing CME with bulk seen predominantly to the southeast in early frames with a very faint, oval-shaped/asymmetric halo shock portion, associated with an X7.1-class flare and associated eruption from AR3842 (S17E18). Coronal signatures include an EUV wave and large-scale dimming in SDO 171/193 with magnetic field line movement off the southern and southeast limbs and dimming of footpoints bridging the Active Region 3842 (S17E18) in GOES 284.
Submitted on 2024-10-02T02:08Z by Chris Stubenrauch

A Notification with ID 20241002-AL-001 was sent on 2024-10-02T02:15Z
A Notification with ID 20241002-AL-002 was sent on 2024-10-02T13:17Z
A Notification with ID 20241003-AL-003 was sent on 2024-10-03T13:17Z

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 SH true SWPC_CAT -10.0 -12.0 963.0 C 60.0 2024-10-02T02:29Z Updated measurement with a lower half-width to try and more closely match the observed type II shock speed for this event of ~1200 km/s. A very approximate analysis based on the fit of the complex-shaped faint shock with two coronagraphs. 1: Result 1 (2.0 AU)
Earth = 2024-10-04T00:37Z
Lucy = 2024-10-04T01:06Z
Mars = 2024-10-05T03:29Z
STEREO A = 2024-10-03T20:30Z
Solar Orbiter = 2024-10-02T18:00Z
2: Result 2 (2.0 AU)
Earth = 2024-10-04T01:18Z
Lucy = 2024-10-04T00:37Z
Mars = 2024-10-05T01:39Z
STEREO A = 2024-10-03T20:22Z
Solar Orbiter = 2024-10-02T18:00Z
3: Result 3 (5.5 AU)
Earth = 2024-10-04T00:41Z
Lucy = 2024-10-03T23:45Z
Mars = 2024-10-05T01:31Z
STEREO A = 2024-10-03T19:52Z
Juno = 2024-10-15T08:00Z
Solar Orbiter = 2024-10-02T18:00Z
Anna Chulaki on 2024-10-02T16:33Z
CME Analysis M2M_CATALOG LE true SWPC_CAT -19.0 -10.0 594.0 C 38.0 2024-10-02T04:22Z Updated bulk measurement based on the best fit between SOHO LASCO C2 and STEREO A COR2 imagery. This event is obscured by the pylon in SOHO LASCO C3 imagery so only early imagery in SOHO LASCO C2 was used in this measurement. Multiple measurements produced speeds ranging from 487 to 632 km/s. 1: Result 1 (2.0 AU)
Earth = 2024-10-04T20:40Z
Lucy = 2024-10-04T19:43Z
Solar Orbiter = 2024-10-03T00:00Z
STEREO A = 2024-10-04T16:30Z
2: Result 2 (5.5 AU)
Earth = 2024-10-04T19:49Z
Lucy = 2024-10-04T18:45Z
Solar Orbiter = 2024-10-03T00:00Z
STEREO A = 2024-10-04T16:30Z
3: Result 3 (2.0 AU)
Earth = 2024-10-04T20:36Z
Lucy = 2024-10-04T19:39Z
4: Result 4 (2.0 AU)
Earth = 2024-10-04T20:19Z
Lucy = 2024-10-04T19:23Z
STEREO A = 2024-10-05T20:44Z
Mattie Anastopulos on 2024-10-02T12:17Z
CME Analysis M2M_CATALOG SH false SWPC_CAT -10.0 -13.0 679.0 C 65.0 2024-10-02T04:09Z Preliminary shock measurement using SOHO C2 early frames capturing the faint and very wide shock; was not able to fit the full shock with half-widths less than 60 degrees given the oval shape. Not modeled Chris Stubenrauch on 2024-10-02T00:22Z
CME Analysis M2M_CATALOG LE false SWPC_CAT -17.0 -5.0 487.0 S 39.0 2024-10-02T05:31Z Preliminary bulk measurement of the CME using only early SOHO C2 frames in a small window from 2024-10-01T23:00Z to 23:36Z and STEREO A COR2 imagery out to 2024-10-02T01:09Z. 1: Result 1 (2.0 AU)
Earth = 2024-10-05T03:32Z
Lucy = 2024-10-05T01:14Z
STEREO A = 2024-10-04T21:00Z
Chris Stubenrauch on 2024-10-02T01:43Z



All directly linked activities:
2024-10-01T21:58:00-FLR-001
FLR Type: X7.1


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