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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-05-16T13:38Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
Activity ID: 2024-05-16T13:38:00-CME-001 (version 1)
Active Region Number: 13664
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
GAP: Data gap
OFL: Outflowing material at the back of the CME
Source Signature Keyword:
OFL: Moving/Opening field lines
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: CME seen to the W in STEREO COR2A, not yet observed in SOHO LASCO due to a lengthy planned data gap that will end at 2024-05-17T02:10Z. The source is far-sided around the west limb, and very likely old AR 3664, estimated to be located around W120 at this time. Best observed as fieldline movement and an EUV wave starting around 2024-05-16T13:34Z in SDO AIA 171/193/211 and GOES SUVI 284.
Submitted on 2024-05-16T16:10Z by Tony
Iampietro
A Notification with ID
20240516-AL-005 was sent on 2024-05-16T17:41Z
A Notification with ID
20240517-AL-001 was sent on 2024-05-17T13:30Z
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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
|
true |
SWPC_CAT |
120.0 |
-2.0 |
1452.0 |
O |
27.0 |
2024-05-16T16:02Z |
Final analysis with two coronagraphs now that SOHO LASCO imagery is available. |
1: Result 1 (2.0 AU)
Mars = 2024-05-19T09:15Z
OSIRIS-APEX = 2024-05-18T08:53Z
Parker Solar Probe = 2024-05-17T22:19Z
Solar Orbiter = 2024-05-18T07:30Z
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Anna Chulaki on 2024-05-17T13:25Z |
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CME Analysis
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M2M_CATALOG |
LE
|
false |
SWPC_CAT |
120.0 |
-2.0 |
1081.0 |
O |
30.0 |
2024-05-16T17:01Z |
Preliminary 3-frame measurement with only available STEREO COR2A data, until SOHO LASCO is available (further analysis will follow). Estimated far-sided longitude of AR 3664 at W120 used, but could range W110-W130. |
1: Result 1 (2.0 AU)
Mars = 2024-05-20T06:40Z
OSIRIS-APEX = 2024-05-18T22:10Z
Parker Solar Probe = 2024-05-18T09:48Z
Solar Orbiter = 2024-05-18T13:00Z
2: Result 2 (5.5 AU)
Mars = 2024-05-20T06:43Z
OSIRIS-APEX = 2024-05-18T22:24Z
Parker Solar Probe = 2024-05-18T09:40Z
Solar Orbiter = 2024-05-18T13:00Z
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Tony Iampietro on 2024-05-16T16:13Z |
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