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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2023-07-10T04:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-07-10T04:00:00-CME-001 (version 1)
Source Location: S13W49
Active Region Number: 13366
Note Keyword:
GAP: Data gap
HAL: Halo CME
PRM: Prominence material (filamentary structures)
Source Signature Keyword:
FLR: Flare
DFLR: Double ribbon flare
FIL: Filament eruption
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: This CME is visible to the SW in SOHO LASCO C2, C3, and STEREO A COR2 imagery (data gap during event in STEREO A as it travels out in the field of view). The source of this CME is a double ribbon flare near AR13366 and plage region 13358 and associated filament eruption starting around 2023-07-10T03:20Z. The eruption is most clearly visible in SDO/AIA 131, 304, and 171. The associated filament is very clearly seen in GOES SUVI 304 as well.
Submitted on 2023-07-10T13:45Z by Carina
Alden
A Notification with ID
20230710-AL-001 was sent on 2023-07-10T15:08Z
A Notification with ID
20230711-AL-001 was sent on 2023-07-11T12:27Z
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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
SH
|
true |
SWPC_CAT |
37.0 |
-10.0 |
901.0 |
C |
45.0 |
2023-07-10T07:48Z |
Based on brightest portion of bulk and shock. Could be argued that this is a full bulk measurement due to the appearance of a wider halo feature later on, however it is not clear if the more central halo is part of this CME, therefore it was excluded from this measurement. |
1: Result 1 (2.0 AU)
Earth = 2023-07-13T00:28Z
(PE: -15.3 h)
OSIRIS-REx = 2023-07-13T11:45Z
Parker Solar Probe = 2023-07-11T09:57Z
STEREO A = 2023-07-12T23:00Z
(PE: -35.5 h)
2: Result 2 (2.0 AU)
Earth = 2023-07-12T23:48Z
(PE: -16.0 h)
OSIRIS-REx = 2023-07-13T10:54Z
Parker Solar Probe = 2023-07-11T10:00Z
STEREO A = 2023-07-12T22:11Z
(PE: -36.3 h)
Solar Orbiter = 2023-07-14T02:00Z
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Carina Alden on 2023-07-10T13:46Z |
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