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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-29T04:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-29T04:00:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
Note: CME first seen to the NW in SOHO LASCO C2 starting at 2024-07-29T04:00Z. Also seen to the NW in SOHO LASCO C3 and to the NW STEREO A COR2. The source of this CME is likely a filament that slowly lifted off the disk near the NW limb starting at ~2024-07-29T03:03Z and is best seen in SDO AIA 304 and SDO AIA 171. The filament can also be seen lifting off the disk in the NW quadrant from the perspective of STEREO A EUVI 195 at ~2024-07-29T03:55Z. The filament loop can be seen in the NW SOHO LASCO C2 prior to the eruption.
Submitted on 2024-07-29T16:04Z by Elizabeth
Juelfs
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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 |
78.0 |
72.0 |
378.0 |
S |
38.0 |
2024-07-29T13:28Z |
Measurement made with running difference imagery from SOHO LASCO C2/C3 and STEREO A COR2 using SWPC_CAT. |
Not modeled
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Elizabeth Juelfs on 2024-07-29T16:06Z |
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