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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-10-02T14:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-10-02T14:24:00-CME-001 (version 1)
Source Location: S18E09
Active Region Number: 13842
Note Keyword:
GAP: Data gap
Source Signature Keyword:
FLR: Flare
Morphology Keyword:
L: Loop
Note: This CME is visible to the S/SE in SOHO LASCO C2/C3 and in a few frames of STEREO A imagery. The source is an eruption and subsequent M3.2 flare from AR 3842 (S18E09) starting around 2024-10-02T13:30Z as seen in SDO AIA 131, 171, 193, 304. There is a data gap in STEREO A COR2 imagery from 2024-10-02T14:08Z to 2024-10-02T17:08Z, in addition to being in campaign mode for the Parker Solar Probe perihelion pass which affects COR2A image quality and cadence.
Submitted on 2024-10-02T23:55Z 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 |
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CME Analysis
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M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-7.0 |
-22.0 |
437.0 |
S |
20.0 |
2024-10-02T21:17Z |
Measurement made using source longitude as seen in UV imagery, as well as best fit using multiple SOHO LASCO C2/C3 frames and only one good frame of STEREO A COR2. There is a data gap in STEREO A COR2 imagery from 2024-10-02T14:08Z to 2024-10-02T17:08Z, in addition to being in campaign mode for the Parker Solar Probe perihelion pass which affects COR2A image quality and cadence. |
1: Result 1 (2.0 AU)
Earth = 2024-10-06T00:00Z
Lucy = 2024-10-06T05:00Z
STEREO A = 2024-10-05T18:00Z
2: Result 2 (2.0 AU)
Earth = 2024-10-04T20:19Z
Lucy = 2024-10-04T19:23Z
STEREO A = 2024-10-05T20:44Z
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Hannah Hermann on 2024-10-02T23:58Z |
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