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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2025-03-28T15:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
STEREO A: SECCHI/COR2
Activity ID: 2025-03-28T15:24:00-CME-001 (version 2)
Source Location: N06E80
Active Region Number: 14046
Note Keyword:
Source Signature Keyword:
FLR: Flare
OFL: Moving/Opening field lines
Morphology Keyword:
Note: This event is visible to the east/northeast in SOHO LASCO C2 and STEREO A COR2 imagery. This CME is still developing and only early imagery is available as a result. The source is related to an eruption and X1.1 flare from Active Region 14046 starting around 2025-03-28T15:00Z as seen in SDO AIA 131, 171, 193, 304 imagery. A subsequent wide opening of field lines can be observed in SDO AIA 171 and 193 imagery at this time as well.
Submitted on 2025-03-28T19:04Z by Mattie
Anastopulos
A Notification with ID
20250328-AL-004 was sent on 2025-03-28T18:55Z
A Notification with ID
20250329-AL-001 was sent on 2025-03-29T00:53Z
A Notification with ID
20250329-AL-002 was sent on 2025-03-29T01:32Z
A Notification with ID
20250330-AL-001 was sent on 2025-03-30T01:59Z
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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 |
SH
|
true |
SWPC_CAT |
-48.0 |
8.0 |
2212.0 |
R |
48.0 |
2025-03-28T17:00Z |
SHOCK measurement based on approximate source location and best fit between SOHO LASCO C2 and STEREO A COR2. This measurement contains a high degree of uncertainty due to the lack of available frames as a result of data gaps in both SOHO and STEREO A COR2. |
1: Result 1 (2.0 AU)
Earth = 2025-03-30T02:32Z
(PE: -31.7 h)
BepiColombo = 2025-03-29T07:19Z
Europa Clipper = 2025-03-31T01:29Z
Lucy = 2025-03-31T07:57Z
Mars = 2025-03-30T18:33Z
OSIRIS-APEX = 2025-03-30T08:00Z
STEREO A = 2025-03-30T17:00Z
2: Result 2 (5.5 AU)
Earth = 2025-03-30T01:51Z
(PE: -32.4 h)
Europa Clipper = 2025-03-30T22:46Z
Lucy = 2025-03-31T05:17Z
Mars = 2025-03-30T16:22Z
BepiColombo = 2025-03-29T06:00Z
OSIRIS-APEX = 2025-03-30T08:00Z
Psyche = 2025-04-03T13:00Z
STEREO A = 2025-03-30T17:00Z
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Mary Aronne on 2025-04-01T13:28Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
-86.0 |
19.0 |
1838.0 |
O |
37.0 |
2025-03-28T17:27Z |
Measurement of the bulk using several more frames of SOHO LASCO C3 imagery than previously available. There is still only one STEREO A COR2 frame available for this CME, but the fit found using C3 frames the source location aligns well with this one STEREO A COR2 frame. |
1: Result 1 (2.0 AU)
Earth = 2025-03-31T10:00Z
(PE: -0.3 h)
OSIRIS-APEX = 2025-03-29T15:05Z
Europa Clipper = 2025-04-01T14:00Z
Lucy = 2025-04-02T12:00Z
Mars = 2025-04-01T04:00Z
2: Result 2 (5.5 AU)
Earth = 2025-03-31T10:00Z
(PE: -0.3 h)
OSIRIS-APEX = 2025-03-29T14:52Z
Europa Clipper = 2025-04-01T14:00Z
Juno = 2025-04-10T03:00Z
Lucy = 2025-04-02T12:00Z
Mars = 2025-04-01T04:00Z
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Hannah Hermann on 2025-03-30T00:15Z |
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CME Analysis
|
M2M_CATALOG |
LE
|
false |
SWPC_CAT |
-81.0 |
20.0 |
1942.0 |
O |
48.0 |
2025-03-28T17:14Z |
Measurement of the brighter BULK portion using only 4 early frames. Measurement based on the approximate source location and best fit between SOHO LASCO C2 and STEREO A COR2 imagery. This measurement contains a high degree of uncertainty due to the lack of available frames as a result of data gaps in both SOHO and STEREO A COR2. |
1: Result 1 (2.0 AU)
Earth = 2025-03-31T04:00Z
(PE: -6.3 h)
Europa Clipper = 2025-03-31T16:18Z
Mars = 2025-03-31T09:42Z
OSIRIS-APEX = 2025-03-29T12:38Z
BepiColombo = 2025-03-29T16:00Z
Lucy = 2025-04-01T10:00Z
2: Result 2 (5.5 AU)
Earth = 2025-03-31T04:00Z
(PE: -6.3 h)
Europa Clipper = 2025-03-31T13:00Z
Mars = 2025-03-31T06:52Z
OSIRIS-APEX = 2025-03-29T12:28Z
BepiColombo = 2025-03-29T16:00Z
Juno = 2025-04-07T06:00Z
Lucy = 2025-04-01T10:00Z
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Melissa Kane on 2025-03-29T01:08Z |
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