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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-03-16T12:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
GOES: CCOR-1
Activity ID: 2026-03-16T12:53:00-CME-001 (version 3)
Source Location: N17E177
Note Keyword:
DFL: Likely deflection of the event within the FOV
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
L: Loop
Note: Bright CME first seen to the NW by STEREO A COR2 beginning at 2026-03-16T12:53Z, as well as by SOHO LASCO C2, C3 and GOES CCOR-1 in later frames. The source of this event is an eruption seen from beyond the NW limb in STEREO A EUVI 195 seen beginning at approx. 2026-03-16T11:55Z. This eruption may have originated from far sided former Active Region 14378 (currently located at approx. N17E177). This CME overlaps in the field of view with Earth directed CME: 2026-03-16T13:26Z.
Version 1 submitted on 2026-03-16T23:27Z by Melissa Kane
Version 2 submitted on 2026-03-17T00:04Z by Melissa Kane
Version 3 submitted on 2026-03-20T16:20Z by Mary Aronne
No Notification has been sent for this activity yet.
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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
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true |
SWPC_CAT |
-177.0 |
40.0 |
380.0 |
S |
34.0 |
2026-03-16T22:01Z |
Measurement based on approximate source location and best fit in SOHO LASCO C2/C3, GOES CCOR-1 and STEREO A COR2. |
1: Result 1 (2.0 AU)
Solar Orbiter = 2026-03-18T04:26Z
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Melissa Kane on 2026-03-16T23:28Z |
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