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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-07-26T15:23Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C3
Activity ID: 2024-07-26T15:23:00-CME-001 (version 1)
Source Location: S08E35
Active Region Number: 13765
Note Keyword:
Faint: Faint event; may affect type assignment
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
DIM: Dimming
Morphology Keyword:
O: Other
Note: Very faint CME seen to the E in SOHO C2/C3, and better in STEREO COR2A until a data gap begins at 2024-07-26T17:09Z. The source for this CME is likely a very broad area of dimming spanning approximately S10E15 to S10E50 observed over the tight cluster of ARs 3767, 3766, 3765, and 3764 beginning around 2024-07-26T13:00Z in SDO AIA 193, appearing centered the most around S08E35 near AR 3765.
Submitted on 2024-07-27T03:33Z 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 |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-37.0 |
0.0 |
328.0 |
S |
38.0 |
2024-07-27T01:21Z |
Measurement made by initially lining up with STEREO COR2A imagery as it is more clear, using the rough center of the dimming ~S08E35 as a start and finding some deflection when triangulating as best as possible with SOHO LASCO C2/C3. Some speculation exists with how faint SOHO observes this CME, and not every frame distinctly sees the front, best seen early in C2 and late in C3. |
1: Result 1 (2.0 AU)
Earth = 2024-07-30T14:00Z
(PE: 14.7 h)
Lucy = 2024-07-31T14:00Z
Parker Solar Probe = 2024-07-29T12:00Z
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 2024-07-27T03:37Z |
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