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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-02-24T06:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-02-24T06:00:00-CME-001 (version 2)
Note Keyword:
DPL: CME exhibits dimpled front
FOV: Front Bright front; may be evidence of pileup
Ha: Bright emission (likely H-alpha emission)
OFL: Outflowing material at the back of the CME
OVR: Event partially overlaps with another CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright, wide CME seen to the NW in SOHO LASCO C2/C3 and STEREO COR2A. Source is seen in SDO AIA 171/193/211 as field line movement beginning around 2025-02-24T04:09Z over the NW limb, with an EUV wave at 2025-02-24T15:18Z, and as a filament liftoff starting around 2025-02-24T05:06Z. The source is better seen in STEREO A EUVI with the filament on/just inside the west limb as viewed from STEREO A. At 2025-02-24T05:15Z, STEREO A was located 30.297 degrees from Earth, putting its west limb around W120.3. Here in STEREO A EUVI 304, the filament can be seen slowly rising starting at 2025-02-24T03:15Z->T5:15Z, and ejecting by the next timestamp at T05:45Z. A post-eruptive arcade follows in STEREO A EUVI 195/304. The source could be, or be near, old AR 3989, which rotated off the west limb on 2025-02-21 and would be located approximately W115-W125.
Submitted on 2025-02-24T17:37Z by Mary
Aronne
A Notification with ID
20250224-AL-003 was sent on 2025-02-24T15:08Z
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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 |
110.0 |
24.0 |
1421.0 |
O |
41.0 |
2025-02-24T08:35Z |
BULK. Triangulated measurement of the brightest bulk portion of the leading edge, notably clipping some of the more faint nose off the northern portion in SOHO C3 imagery due to the uneven front. This analysis may be preliminary as further analysis continues. |
1: Result 1 (2.0 AU)
Juice = 2025-02-25T14:18Z
Parker Solar Probe = 2025-02-25T15:00Z
2: Result 2 (2.0 AU)
Juice = 2025-02-25T07:17Z
Parker Solar Probe = 2025-02-25T14:00Z
STEREO A = 2025-02-26T12:00Z
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Tony Iampietro on 2025-02-24T14:51Z |
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All directly linked activities: |
| No Linked Activity Found. |
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