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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-03-07T22:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-03-07T22:36:00-CME-001 (version 1)
Source Location: N15W90
Note Keyword:
GAP: Data gap
Source Signature Keyword:
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: This CME is visible to the northwest in SOHO LASCO C2/C3 imagery and is seen for a few frames in STEREO A COR2 following a data gap from 2024-03-07T16:53Z to 2024-03-05T03:23Z. The source is a filament eruption visible on the northwest limb centered around N15W90 which begins to lift-off at 2024-03-07T22:10Z as seen in SDO AIA 304. An opening of field lines can be seen in SDO AIA 171 and 193 imagery with post eruptive arcades visible in SDO AIA 171, 193, and 304 starting around 2024-03-07T23:30Z.
Submitted on 2024-03-08T14:54Z by Mattie
Anastopulos
A Notification with ID
20240308-AL-001 was sent on 2024-03-08T18:48Z
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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
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true |
SWPC_CAT |
95.0 |
40.0 |
557.0 |
C |
40.0 |
2024-03-08T05:08Z |
Measurement of the leading edge using an approximated longitude of W95 based on available UV imagery. The leading edge becomes too diffuse to track about halfway through the SOHO LASCO C3 field of view. No difference imagery from STEREO A COR2 was used in this measurement, since the leading edge was already outside the STEREO A COR2 field of view in available frames, after a data gap that lasted from 2024-03-07T17:09Z to 2024-03-08T03:09Z. |
1: Result 1 (2.0 AU)
Mars = 2024-03-13T00:00Z
OSIRIS-APEX = 2024-03-11T01:00Z
2: Result 2 (2.0 AU)
Mars = 2024-03-13T03:00Z
OSIRIS-APEX = 2024-03-11T03:00Z
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Hannah Hermann on 2024-03-08T16:51Z |
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