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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-15T08:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-05-15T08:36:00-CME-001 (version 1)
Source Location: S15W90
Active Region Number: 13664
Note Keyword:
3P: 3-part structure CME
DFL: Likely deflection of the event within the FOV
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Bright CME seen due West in SOHO LASCO C2/C3 and STEREO A COR2. Source is EUV wave seen beyond the SW limb starting at 2024-05-15T08:18Z in SDO AIA 171/193. Widely opening field lines with northern deflection seen on or just beyond the SW limb at an apparent latitude of S15 (before deflection). This CME overlaps heavily with CME: 2024-05-15T08:48Z.
Submitted on 2024-05-15T13:46Z by Hannah
Hermann
A Notification with ID
20240515-AL-009 was sent on 2024-05-15T17:09Z
A Notification with ID
20240516-AL-001 was sent on 2024-05-16T02:22Z
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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
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
105.0 |
2.0 |
1766.0 |
O |
31.0 |
2024-05-15T10:33Z |
Measurement of the BULK using candidate source location AR 13664 approximated longitude of W105, and best fit between coronagraphs. |
1: Result 1 (2.0 AU)
Mars = 2024-05-18T01:36Z
OSIRIS-APEX = 2024-05-17T02:40Z
Parker Solar Probe = 2024-05-16T16:43Z
2: Result 2 (5.5 AU)
Mars = 2024-05-18T01:57Z
OSIRIS-APEX = 2024-05-17T02:44Z
Parker Solar Probe = 2024-05-16T17:07Z
3: Result 3 (2.0 AU)
Mars = 2024-05-17T15:40Z
OSIRIS-APEX = 2024-05-16T22:20Z
Parker Solar Probe = 2024-05-16T10:57Z
Solar Orbiter = 2024-05-17T04:00Z
4: Result 4 (2.0 AU)
Mars = 2024-05-17T14:19Z
OSIRIS-APEX = 2024-05-16T21:02Z
Parker Solar Probe = 2024-05-16T10:50Z
Solar Orbiter = 2024-05-17T04:00Z
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Hannah Hermann on 2024-05-15T13:48Z |
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