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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-05-02T11:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2026-05-02T11:24:00-CME-001 (version 1)
Note Keyword:
DFL: Likely deflection of the event within the FOV
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
Morphology Keyword:
Note: CME first seen to the WNW in SOHO LASCO C2 starting at 2026-05-02T11:24Z. It is also seen to the WNW in SOHO LASCO C3, GOES CCOR-1, and faintly for a couple frames in STEREO A COR2. The source of this CME is most likely a filament eruption centered around N16W75 to the W of AR 14424. The eruption is best seen in SDO AIA 304 and STEREO A SUVI 304 beginning around 2026-05-02T10:48Z. The eruption is also associated with a C4.0 flare that peaked at 2026-05-02T11:04Z and was centered around N16W75. There appears to be some minor southward deflection later in the propagation of the CME. There is likely also some westward deflection due to the proximity to a coronal hole that was centered at approximately N33W30 at the time of the eruption.
Version 1 submitted on 2026-05-02T14:39Z by Elizabeth Juelfs
A Notification with ID
20260502-AL-001 was sent on 2026-05-02T16:39Z
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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 |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
92.0 |
16.0 |
603.0 |
C |
20.0 |
2026-05-02T17:18Z |
Measurement based on triangulated best fit among SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2. There is some degree of uncertainty in this measurement because this CME is partially obscured by a brighter CME in STEREO A COR2. |
1: Result 1 (2.0 AU)
Parker Solar Probe = 2026-05-04T16:21Z
STEREO A = 2026-05-06T00:00Z
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Elizabeth Juelfs on 2026-05-02T14:45Z |
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