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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-01-20T09:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-01-20T09:24:00-CME-001 (version 2)
Source Location: S15E15
Note Keyword:
DFL: Likely deflection of the event within the FOV
HAL: Halo CME
OVR: Event partially overlaps with another CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
Morphology Keyword:
LS: Loop and Shock Candidate
Note: Partial halo CME seen to the south/southeast in SOHO LASCO C2/C3 and STEREO A COR2. Source is a filament eruption on the Earth-facing disk stretching from S15E00 to S15E35, with liftoff starting around 2024-01-20T08:27Z. Liftoff of material and post-eruptive brightening can be seen in SDO AIA 304 at 2024-01-20T08:27Z. Opening field lines seen in SDO AIA 171 and dimming seen in SDO AIA 193 starting at 2024-01-20T08:39Z - dimming spans from S20 up to N10; from E05 to E40. Posts-eruptive arcades seen in SDO AIA 171/193 and STEREO A EUVI 195 forming at 2024-01-20T09:13Z. This eruption can also be seen in STEREO A EUVI 304 imagery as brightening and ejecta, and in STEREO A EUVI 195 imagery as dimming and post-eruptive arcades. This CME overlaps with another filament eruption on the NE limb which resulted in CME:2024-01-20T09:36Z.
Submitted on 2024-01-20T16:03Z by Hannah
Hermann
A Notification with ID
20240120-AL-001 was sent on 2024-01-20T17:15Z
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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 |
-18.0 |
-22.0 |
978.0 |
C |
47.0 |
2024-01-20T12:49Z |
Measurement of irregular leading edge. Measurement made using source location as seen in UV imagery and best fit between coronagraphs. This CME overlaps with a simultaneous CME seen to the northeast, making it a bit difficult to distinguish the northern portion of the leading edge in difference imagery. This adds some uncertainty to the measurement. |
1: Result 1 (2.0 AU)
Earth = 2024-01-22T13:19Z
(PE: -2.7 h)
Psyche = 2024-01-23T19:20Z
Solar Orbiter = 2024-01-22T12:09Z
STEREO A = 2024-01-22T11:24Z
(PE: -13.4 h)
2: Result 2 (5.5 AU)
Earth = 2024-01-22T13:23Z
(PE: -2.6 h)
Solar Orbiter = 2024-01-22T11:57Z
STEREO A = 2024-01-22T11:21Z
(PE: -13.5 h)
Juno = 2024-02-06T00:00Z
3: Result 3 (2.0 AU)
Earth = 2024-01-22T12:56Z
(PE: -3.1 h)
Psyche = 2024-01-23T19:35Z
Solar Orbiter = 2024-01-22T12:56Z
STEREO A = 2024-01-22T10:57Z
(PE: -13.9 h)
4: Result 4 (5.5 AU)
Earth = 2024-01-22T13:01Z
(PE: -3.0 h)
Solar Orbiter = 2024-01-22T12:39Z
STEREO A = 2024-01-22T10:54Z
(PE: -13.9 h)
Psyche = 2024-01-23T19:45Z
Juno = 2024-02-06T22:00Z
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Hannah Hermann on 2024-01-20T16:26Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
false |
SWPC_CAT |
-20.0 |
-11.0 |
1088.0 |
O |
49.0 |
2024-01-20T12:06Z |
Shock measurement using source location seen in UV imagery and best fit between coronagraphs. This shock front has a slightly asymmetrical shape. There is inherent uncertainty in this measurement due to the head-on directionality of the CME (i.e. being a partial halo). |
1: Result 1 (2.0 AU)
Earth = 2024-01-22T08:25Z
(PE: -7.6 h)
Psyche = 2024-01-23T11:29Z
Solar Orbiter = 2024-01-22T07:09Z
STEREO A = 2024-01-22T06:37Z
(PE: -18.2 h)
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Hannah Hermann on 2024-01-20T15:23Z |
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