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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-04-21T11:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-04-21T11:12:00-CME-001 (version 1)
Source Location: S17W34
Active Region Number: 13638
Note Keyword:
Faint: Faint event; may affect type assignment
GAP: Data gap
Source Signature Keyword:
FLR: Flare
BR: Brightening
Morphology Keyword:
J: Jet
Note: Very faint and narrow CME seen to the SW in SOHO LASCO C2/C3. Source is likely a small flare and narrow ejecta from S17W34 (near AR 3638) at 2024-04-21T10:51Z as seen in SDO AIA 304, at 10:49Z in GOES SUVI 304. Small patch of brightening seen at source location in STEREO A EUVI 195 at 10:55Z; lingering narrow ejecta material seen in STEREO A EUVI 304 at 11:15Z. Data gap in STEREO A COR2 lasting from 2024-04-21T11:38Z to 2024-04-22T02:23Z (with one frame timestamped 2024-04-2119:23Z). No STEREO A COR2 imagery was available for this CME.
Submitted on 2024-04-22T20:06Z by Hannah
Hermann
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) |
Submitted By |
CME Analysis
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M2M_CATALOG |
LE
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true |
SWPC_CAT |
28.0 |
-43.0 |
687.0 |
C |
19.0 |
2024-04-21T16:13Z |
Measurement of faint leading edge using source location with heavy deflection to the south and to more central longitudes (corroborated by apparent trajectory of material seen in 304 UV imagers). Data gap in STEREO A COR2 lasting from 2024-04-21T11:38Z to 2024-04-22T02:23Z (with one frame timestamped 2024-04-2119:23Z). No STEREO A imagery was available for this CME. |
Not modeled
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Hannah Hermann on 2024-04-22T20:08Z |
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