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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-02-15T09:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-02-15T09:24:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
HAL: Halo CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
F: Flux Rope
Note: Halo CME seen to the South in SOHO LASCO C2/C3 and STEREO A COR2. Source is rising loop and widely opening field lines seen beyond S limb starting at 2024-02-15T09:06Z in SDO AIA 171, GOES SUVI 193/284/304. EUV wave seen extending to about S55 on the Earth-facing disk in SDO AIA 193 and GOES SUVI 195. Additional outflow seen emerging from beyond the S limb in SDO AIA 171 at 09:21Z.
Submitted on 2024-02-15T14:53Z by Hannah
Hermann
A Notification with ID
20240215-AL-001 was sent on 2024-02-15T16:44Z
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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 |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
-173.0 |
-22.0 |
1953.0 |
O |
45.0 |
2024-02-15T11:06Z |
Measurement using best fit between coronagraphs. Tricky fit in STEREO A COR2. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2024-02-16T10:22Z
2: Result 2 (5.5 AU)
Parker Solar Probe = 2024-02-16T10:23Z
Juno = 2024-03-04T06:00Z
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Hannah Hermann on 2024-02-15T14:54Z |
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No Linked Activity Found. |
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