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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-04-26T07:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2025-04-26T07:36:00-CME-001 (version 1)
Source Location: N00W123
Note Keyword:
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
L: Loop
Note: Loop CME visible to the W in SOHO LASCO C2, C3, and W in STEREO A COR2. Source is an eruption beyond the W limb, with opening field lines and ejecta located at about N00W123 as seen in STEREO A EUVI 304 and 195, starting at 2025-04-26T07:05Z.
Submitted on 2025-04-26T13:25Z by Hannah
Hermann
A Notification with ID
20250426-AL-001 was sent on 2025-04-26T14:50Z
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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 |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
126.0 |
-7.0 |
645.0 |
C |
26.0 |
2025-04-26T12:39Z |
Measurement using best fit between several frames of SOHO LASCO C2, C3, and STEREO A COR2, as well as source location seen in UV imagery. |
1: Result 1 (2.0 AU)
BepiColombo = 2025-04-27T10:00Z
Juice = 2025-04-29T04:00Z
Parker Solar Probe = 2025-04-28T00:00Z
Solar Orbiter = 2025-04-27T20:00Z
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Hannah Hermann on 2025-04-26T14:25Z |
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All directly linked activities: |
No Linked Activity Found. |
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Comments by users: |
0 comment received. |
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