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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-02-06T02:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-02-06T02:53:00-CME-001 (version 3)
Source Location: S34W65
Active Region Number: 13575
Note Keyword:
3P: 3-part structure CME
DFL: Likely deflection of the event within the FOV
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
HAL: Halo CME
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Source of this partial halo CME is an M2.2 class flare from AR 3575 (S34W65) peaked at 2024-02-06T02:28Z and followed by an M4.2 class flare. The flare was associated with a large eruption seen in SDO AIA 193/304/171/131 and STEREO EUVI 195 starting at 2024-02-06T02:13Z (ejecta, EUV wave, post-eruptive arcades and circular dimming around them and rising).
Submitted on 2024-02-06T15:29Z by Mary
Aronne
A Notification with ID
20240206-AL-002 was sent on 2024-02-06T14:46Z
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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 |
SH
|
true |
SWPC_CAT |
48.0 |
-45.0 |
857.0 |
C |
52.0 |
2024-02-06T06:32Z |
This is a measurement of the wider, faster, fainter shock of the CME, not the leading edge/bulk of the CME. This portion of the CME extends further to the east in coronagraph imagery compared to the bulk. |
1: Result 1 (2.0 AU)
Earth = 2024-02-09T08:00Z
(PE: -13.7 h)
OSIRIS-APEX = 2024-02-08T06:00Z
STEREO A = 2024-02-09T00:00Z
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Mary Aronne on 2024-02-06T13:56Z |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
62.0 |
-48.0 |
772.0 |
C |
43.0 |
2024-02-06T07:11Z |
This is a measurement of the leading edge of the CME, encompassing the bulk of the CME. Longitude based on source location, and best fit between coronagraphs in SWPC_CAT. |
1: Result 1 (2.0 AU)
OSIRIS-APEX = 2024-02-08T06:00Z
2: Result 2 (5.5 AU)
Lucy = 2024-02-13T00:00Z
OSIRIS-APEX = 2024-02-08T06:00Z
3: Result 3 (2.0 AU)
OSIRIS-APEX = 2024-02-08T00:00Z
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Mary Aronne on 2024-02-06T13:55Z |
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CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
65.0 |
-56.0 |
698.0 |
C |
47.0 |
2024-02-06T07:39Z |
Preliminary measurement using limited frames of STEREO A COR2. |
Not modeled
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Mary Aronne on 2024-02-06T13:43Z |
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