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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-01-08T05:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2026-01-08T05:53:00-CME-001 (version 1)
Source Location: S18E05
Active Region Number: 14334
Note Keyword:
Source Signature Keyword:
FLR: Flare
Morphology Keyword:
Note: This CME is visible to the southeast in SOHO LASCO C2/C3, GOES CCOR-1, and STEREO A COR2 imagery. This event is more narrow as observed by STEREO A COR2 imagery, while a wider feature is observed in SOHO LASCO C2/C3 and GOES CCOR-1. The source is an eruption and C4.4 flare from Active Region 14334 (S18E05) starting around 2026-01-08T05:30Z as seen in SDO AIA 131/171/193/304, GOES SUVI 131/171/195/284/304 and STEREO A EUVI 195/304 imagery. Ejecta can be observed deflecting southeast of the eruption site, possibly due to a nearby coronal hole west of AR 14334.
Version 1 submitted on 2026-01-08T13:24Z by Mattie Anastopulos
A Notification with ID
20260108-AL-001 was sent on 2026-01-08T14:30Z
A Notification with ID
20260109-AL-002 was sent on 2026-01-09T03:34Z
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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 |
-10.0 |
-35.0 |
1016.0 |
O |
35.0 |
2026-01-08T08:49Z |
Measurement following the wider feature seen in SOHO LASCO imagery. The measured parameters were obtained between the approximate source location and best fit between SOHO LASCO C3 and STEREO A COR2 imagery. |
1: Result 1 (2.0 AU)
Earth = 2026-01-10T10:15Z
(PE: -9.3 h)
Solar Orbiter = 2026-01-09T23:52Z
OSIRIS-APEX = 2026-01-10T08:00Z
STEREO A = 2026-01-11T07:00Z
(PE: 4.0 h)
2: Result 2 (5.5 AU)
Earth = 2026-01-10T09:48Z
(PE: -9.8 h)
Solar Orbiter = 2026-01-09T23:30Z
Juno = 2026-01-23T00:00Z
OSIRIS-APEX = 2026-01-10T08:00Z
STEREO A = 2026-01-11T07:00Z
(PE: 4.0 h)
3: Result 3 (2.0 AU)
Earth = 2026-01-10T09:19Z
(PE: -10.3 h)
OSIRIS-APEX = 2026-01-10T14:27Z
Solar Orbiter = 2026-01-09T23:36Z
STEREO A = 2026-01-11T07:00Z
(PE: 4.0 h)
4: Result 4 (5.5 AU)
Earth = 2026-01-10T09:08Z
(PE: -10.5 h)
OSIRIS-APEX = 2026-01-10T14:07Z
Solar Orbiter = 2026-01-09T23:31Z
Juno = 2026-01-22T20:00Z
STEREO A = 2026-01-11T07:00Z
(PE: 4.0 h)
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Mattie Anastopulos on 2026-01-08T13:27Z |
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