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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-26T21:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-26T21:24:00-CME-001 (version 1)
Source Location: S22W05
Active Region Number: 13762
Note Keyword:
COL: Possible collision with previous CME
DFL: Likely deflection of the event within the FOV
Faint: Faint event; may affect type assignment
GAP: Data gap
HAL: Halo CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
O: Other
Note: Faint partial halo seen to the S in both coronagraphs, although STEREO COR2A resumes from a data gap at 2024-07-26T22:38Z. The source for this is likely an eruption from AR 3672 centered around S22W05, observed in SDO AIA 193 starting around 2024-07-26T19:38Z. This event is closely preceded by CME 2024-07-26T20:48Z, also from AR 3672, which tracks separately from this front.
Submitted on 2024-07-27T05:48Z by Tony
Iampietro
A Notification with ID
20240727-AL-001 was sent on 2024-07-27T06:23Z
A Notification with ID
20240727-AL-004 was sent on 2024-07-27T20:54Z
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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 |
-1.0 |
-5.0 |
646.0 |
C |
20.0 |
2024-07-27T00:52Z |
Triangulated measurement between SOHO and STEREO, with good confidence in this fit compared to the outermost front of preceding CME 26/20:48Z, as this front appears much brighter in SOHO and STEREO coronagraph imagery following that separate front. |
1: Result 1 (2.0 AU)
Earth = 2024-07-30T00:06Z
(PE: 0.8 h)
Parker Solar Probe = 2024-07-28T17:49Z
Lucy = 2024-07-31T09:00Z
STEREO A = 2024-07-29T15:00Z
(PE: -4.2 h)
2: Result 2 (2.0 AU)
Earth = 2024-07-29T15:44Z
(PE: -7.6 h)
Lucy = 2024-07-30T20:34Z
Parker Solar Probe = 2024-07-28T14:07Z
STEREO A = 2024-07-29T10:16Z
(PE: -8.9 h)
3: Result 3 (2.0 AU)
Earth = 2024-07-29T13:38Z
(PE: -9.7 h)
Lucy = 2024-07-30T19:43Z
Parker Solar Probe = 2024-07-28T14:01Z
STEREO A = 2024-07-29T08:51Z
(PE: -10.4 h)
Mars = 2024-08-01T06:00Z
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Tony Iampietro on 2024-07-27T05:49Z |
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