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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-02-14T04:09Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-02-14T04:09:00-CME-001 (version 2)
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Partial halo CME directed to the SW in SOHO LASCO C2/C3 and STEREO A COR2. The source is believed to be on the far side, as an opening field lines and an EUV wave visible in SDO AIA 171 starting at 2024-02-14T03:51Z. EUV wave is best seen in SDO AIA 193 and GOES SUVI 284. The eruption is faintly seen in STEREO A EUV 195 beyond the SW limb. A possible candidate Active Region is AR 3575, which rotated off of the Earth-facing disk on 2024-02-07 and produced several M-class flares during its time on the disk.
Submitted on 2025-02-06T21:19Z by Mary
Aronne
A Notification with ID
20240214-AL-003 was sent on 2024-02-14T16:22Z
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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
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true |
SWPC_CAT |
168.0 |
-38.0 |
2012.0 |
R |
43.0 |
2024-02-14T05:45Z |
Measurement of leading edge using SOHO LASCO C3 and STEREO A COR2. The bulk of the CME is wider than the shock, which extends to almost a full halo in the coronagraphs. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-02-15T11:00Z
Mars = 2024-02-17T01:00Z
OSIRIS-APEX = 2024-02-15T16:00Z
2: Result 2 (5.5 AU)
Parker Solar Probe = 2024-02-15T11:18Z
Mars = 2024-02-17T01:00Z
OSIRIS-APEX = 2024-02-15T16:00Z
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Mary Aronne on 2024-02-14T16:46Z |
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CME Analysis
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M2M_CATALOG |
SH
|
true |
SWPC_CAT |
173.0 |
-12.0 |
2544.0 |
R |
45.0 |
2024-02-14T05:10Z |
Measurement of the wider, faster, fainter shock of the CME. |
1: Result 1 (2.0 AU)
Mars = 2024-02-16T07:05Z
OSIRIS-APEX = 2024-02-15T05:33Z
Parker Solar Probe = 2024-02-15T00:47Z
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Mary Aronne on 2024-02-14T16:46Z |
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All directly linked activities: |
| No Linked Activity Found. |
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