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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-03-08T04:17Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-03-08T04:17:00-CME-001 (version 1)
Note Keyword:
3P: 3-part structure CME
COL: Possible collision with previous CME
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
BR: Brightening
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: CME with an irregular front seen to the NW in SOHO LASCO C2/C3 and STEREO A COR2. Source is a fast eruption from beyond the NW limb with an apparent latitude of N25, possibly about W110-120, first seen at 2024-03-08T03:40Z in SDO AIA 171/193/304 and GOES SUVI 284/304. Seen in SDO AIA 171/193 as ejecta and some minor field line movement. Seen in SDO AIA 304 as ejecta and a bright ribbon of material. Seen in GOES SUVI 304/284 as opening field lines and bright ejecta, with a ribbon seen in 304.
Submitted on 2024-03-08T19:43Z by Hannah
Hermann
A Notification with ID
20240308-AL-002 was sent on 2024-03-08T20:18Z
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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 |
110.0 |
37.0 |
639.0 |
C |
45.0 |
2024-03-08T09:01Z |
Measurement based on the best fit between SOHO LASCO C3 and STEREO A COR2 imagery. Since the source is far-sided and a precise source longitude is unknown, the measured longitude may vary by +/- 10 degrees. |
1: Result 1 (2.0 AU)
Mars = 2024-03-12T17:04Z
OSIRIS-APEX = 2024-03-10T20:27Z
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Mattie Anastopulos on 2024-03-08T19:53Z |
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No Linked Activity Found. |
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