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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-12-29T06:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-12-29T06:24:00-CME-001 (version 1)
Source Location: S17E30
Active Region Number: 13939
Note Keyword:
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
DIM: Dimming
Morphology Keyword:
Note: This CME is visible to the southeast in STEREO A COR2 and as a partial halo directed towards the southeast in SOHO LASCO C2/C3 imagery. The source is likely related to an eruption and subsequent M2.0 flare from from Active Region 13939 (S17E30) starting around 2024-12-29T04:40Z as seen in GOES SUVI 131, 171, 195, 284, 304 imagery. A subsequent dimming is observed around the eruption site in GOES SUVI 195 imagery at this time as well.
Submitted on 2024-12-29T15:01Z by Mattie
Anastopulos
A Notification with ID
20241229-AL-006 was sent on 2024-12-29T16:29Z
A Notification with ID
20241230-AL-001 was sent on 2024-12-30T00:09Z
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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
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-20.0 |
-21.0 |
860.0 |
C |
45.0 |
2024-12-29T10:14Z |
Measurement of the brighter, bulk portion of this event based on the approximate source location and best fit between SOHO LASCO C3 and STEREO A COR2 imagery. |
1: Result 1 (2.0 AU)
Earth = 2024-12-31T13:14Z
(PE: -2.5 h)
Europa Clipper = 2025-01-01T11:40Z
Lucy = 2024-12-31T20:21Z
Mars = 2025-01-02T15:17Z
Solar Orbiter = 2024-12-31T09:22Z
STEREO A = 2025-01-01T01:22Z
(PE: 0.0 h)
Juice = 2024-12-31T05:00Z
2: Result 2 (5.5 AU)
Earth = 2024-12-31T13:11Z
(PE: -2.5 h)
Europa Clipper = 2025-01-01T11:36Z
Lucy = 2024-12-31T20:17Z
Mars = 2025-01-02T15:08Z
Solar Orbiter = 2024-12-31T09:15Z
STEREO A = 2025-01-01T01:20Z
(PE: 0.0 h)
Juice = 2024-12-31T05:00Z
Juno = 2025-01-13T18:00Z
3: Result 3 (2.0 AU)
Earth = 2024-12-31T10:28Z
(PE: -5.3 h)
Europa Clipper = 2025-01-01T08:56Z
Lucy = 2024-12-31T16:59Z
Mars = 2025-01-02T08:52Z
Solar Orbiter = 2024-12-31T10:12Z
STEREO A = 2025-01-01T00:31Z
(PE: -0.8 h)
Juice = 2024-12-31T04:00Z
4: Result 4 (5.5 AU)
Earth = 2024-12-31T10:29Z
(PE: -5.2 h)
Europa Clipper = 2025-01-01T08:59Z
Lucy = 2024-12-31T16:52Z
Mars = 2025-01-02T08:55Z
Solar Orbiter = 2024-12-31T10:13Z
STEREO A = 2025-01-01T00:31Z
(PE: -0.8 h)
Juice = 2024-12-31T04:00Z
Juno = 2025-01-12T18:00Z
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Mattie Anastopulos on 2024-12-29T16:41Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-20.0 |
-26.0 |
1114.0 |
O |
45.0 |
2024-12-29T09:13Z |
Measurement of the faint, outermost SHOCK feature based on the source location and best fit between SOHO LASCO C3 and STEREO A COR2 imagery. |
1: Result 1 (2.0 AU)
Earth = 2024-12-31T06:14Z
(PE: -9.5 h)
Europa Clipper = 2025-01-01T03:47Z
Lucy = 2024-12-31T12:50Z
Mars = 2025-01-02T06:04Z
Solar Orbiter = 2024-12-31T02:54Z
STEREO A = 2024-12-31T19:41Z
(PE: -5.7 h)
2: Result 2 (5.5 AU)
Earth = 2024-12-31T06:26Z
(PE: -9.3 h)
Europa Clipper = 2025-01-01T03:53Z
Lucy = 2024-12-31T12:58Z
Mars = 2025-01-02T06:11Z
Solar Orbiter = 2024-12-31T02:53Z
STEREO A = 2024-12-31T19:58Z
(PE: -5.4 h)
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Mattie Anastopulos on 2024-12-29T16:40Z |
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