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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2022-04-02T13:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2022-04-02T13:38:00-CME-001 (version 3)
Source Location: N15W61
Active Region Number: 12976
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
Ha: Bright emission (likely H-alpha emission)
PRM: Prominence material (filamentary structures)
SEP: Solar Energetic Particle event
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
Note: Large CME seen to the west in STEREO A COR2, in SOHO LASCO C2, and C3. The source of this CME is a flare from AR12976 and associated filament eruption. EUV wave is visible in SDO/AIA 171, 211, 193, and STEREO A EUVI 195. The eruption begins around 13:00Z. | Note: the associated AR has been updated after further analysis of the event.
Submitted on 2022-04-11T18:04Z by Michelangelo
Romano
A Notification with ID
20220402-AL-005 was sent on 2022-04-02T17:38Z
A Notification with ID
20220403-AL-001 was sent on 2022-04-03T12:46Z
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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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME |
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
SH
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true |
SWPC_CAT |
54.0 |
-15.0 |
1370.0 |
O |
45.0 |
2022-04-02T16:12Z |
Bulk CME measurement based off of matching features seen in SOHO LASCO C3 and STEREO A COR2. There are parts of this CME that are more northern that were not included in this measurement. A best fit based off of the shock and leading edge features was used for these parameters. |
1: Result 1 (2.0 AU)
Earth = 2022-04-04T16:00Z
Mars = 2022-04-05T05:44Z
OSIRIS-REx = 2022-04-04T22:04Z
Solar Orbiter = 2022-04-03T09:15Z
STEREO B = 2022-04-04T10:13Z
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Carina Alden on 2022-04-02T16:53Z |
CME Analysis
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M2M_CATALOG |
SH
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false |
SWPC_CAT |
73.0 |
-11.0 |
1328.0 |
O |
45.0 |
2022-04-02T16:19Z |
Very preliminary measurement based off of a few frames in STEREO A COR2, SOHO LASCO C2 and C3. Updated parameters will be available as more imagery comes in. |
Not modeled
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Carina Alden on 2022-04-02T14:50Z |
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Comments by users: |
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