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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-06-10T19:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
GOES: CCOR-1
Activity ID: 2025-06-10T19:00:00-CME-001 (version 1)
Source Location: N17E90
Note Keyword:
DFL: Likely deflection of the event within the FOV
Source Signature Keyword:
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
O: Other
Note: CME observed to the northeast in SOHO LASCO C2/C3, GOES CCOR-1, and faintly in a few frames of STEREO A COR2. The source is an unnumbered active region on the northeast limb, observed here as filament ejecta in SDO AIA 304 starting around 2025-06-10T18:42Z, originating from around N17E90 where it then more widely fans out. Also observed as field line movement in SDO AIA 171 at this time.
Version 1 submitted on 2025-06-11T00:20Z by Tony Iampietro
A Notification with ID
20250611-AL-002 was sent on 2025-06-11T02:33Z
A Notification with ID
20250611-AL-003 was sent on 2025-06-11T12:31Z
A Notification with ID
20250611-AL-004 was sent on 2025-06-11T19:18Z
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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
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-85.0 |
25.0 |
685.0 |
C |
29.0 |
2025-06-10T23:38Z |
Triangulated measurement between later frames of SOHO LASCO C3 and two available, low quality running difference images of STEREO A COR2. The CME deflects northward as it travels through LASCO C2 to C3 so later frames capture the final width and direction better. STEREO A COR2 imagery becomes sparse over this CME leading to lower quality running difference imagery that is usable. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-06-11T16:39Z
Mars = 2025-06-15T01:00Z
2: Result 2 (5.5 AU)
BepiColombo = 2025-06-11T16:25Z
Europa Clipper = 2025-06-16T16:00Z
Lucy = 2025-06-17T16:00Z
Mars = 2025-06-15T00:00Z
3: Result 3 (2.0 AU)
BepiColombo = 2025-06-11T16:51Z
Mars = 2025-06-15T00:00Z
4: Result 4 (5.5 AU)
BepiColombo = 2025-06-11T16:37Z
Europa Clipper = 2025-06-16T12:00Z
Lucy = 2025-06-17T14:00Z
Mars = 2025-06-15T00:00Z
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Tony Iampietro on 2025-06-11T00:22Z |
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