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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-08-06T07:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2025-08-06T07:24:00-CME-001 (version 2)
Source Location: N05W15
Active Region Number: 14168
Note Keyword:
DFL: Likely deflection of the event within the FOV
Faint: Faint event; may affect type assignment
Source Signature Keyword:
FLR: Flare
BR: Brightening
DIM: Dimming
Morphology Keyword:
Note: CME visible to the west in SOHO LASCO C2/C3 and GOES CCOR-1. Not clearly visible in STEREO A COR2. The potential source is a C5.2 flare and eruption from AR 4168 (approximately N05W15) starting at 2025-08-06T06:04Z, best seen in GOES SUVI 195 and 284.
Version 1 submitted on 2025-08-06T15:30Z by Mary Aronne
Version 2 submitted on 2025-08-06T15:41Z by Mary Aronne
A Notification with ID
20250806-AL-002 was sent on 2025-08-06T17:37Z
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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) |
Measured On |
Submitted By |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
32.0 |
10.0 |
747.0 |
C |
13.0 |
2025-08-06T11:01Z |
Measurement based on best fit with SOHO LASCO C2/C3 and GOES CCOR-1 in SWPC_CAT focusing on measuring the northernmost portion of the leading edge. The CME may deflect west from the source location. This CME measurement is more approximate than usual, due to lack of visibility in STEREO A COR2 imagery. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-08-07T02:00Z
OSIRIS-APEX = 2025-08-08T18:00Z
Parker Solar Probe = 2025-08-08T00:00Z
STEREO A = 2025-08-08T20:00Z
(PE: -3.0 h)
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2025-08-06T15:41Z |
Mary Aronne on 2025-08-06T15:41Z |
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