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Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2026-06-30T21:45Z ( GOES: CCOR-1 )
All Detecting Spacecrafts:
GOES: CCOR-1
Activity ID: 2026-06-30T21:45:00-CME-001 (version 1)
Source Location: N17W18
Active Region Number: 14479
Note Keyword:
GAP: Data gap
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
DFLR: Double ribbon flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
Note: Full halo CME currently observed only in GOES CCOR-1 and somewhat blocked by its pylon. Not yet observed in other coronagraphs due to a SOHO LASCO DSN gap between 2026-06-30T20:15Z to 2026-06-30T23:45Z, and STEREO A data gap starting at 2026-06-30T19:23Z. The source is associated with an X1.1 flare (N17W18) observed in SDO AIA 131 from AR 14479 (N16W22), peaking at 2026-06-30T20:50Z. Also observed as a NE-deflected EUV wave and wide swath of dimming in SDO AIA 193/211 centered around N20W05, brightening/flare ribbons along a channel to the NE of the region in SDO AIA 131/171/193/211/304, and a post-eruptive brightening starting around 2026-06-30T21:46Z.
Version 1 submitted on 2026-06-30T22:52Z by Tony Iampietro
A Notification with ID
20260630-AL-008 was sent on 2026-06-30T23:37Z
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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) |
Measured On |
Submitted By |
|
CME Analysis
|
M2M_CATALOG |
LE
|
true |
SWPC_CAT |
1.0 |
18.0 |
965.0 |
C |
41.0 |
2026-07-01T00:32Z |
Preliminary bulk anaylsis with only several available GOES CCOR-1 frames. Due to the limited frames and full halo presentation, the CME width could vary, impacting speed. Current preliminary analysis of the bulk is consistently around 900-1000 km/s, with high confidence in the latitude and longitude. |
1: Result 1 (2.0 AU)
Earth = 2026-07-03T03:59Z
BepiColombo = 2026-07-01T21:34Z
Europa Clipper = 2026-07-04T21:32Z
Juice = 2026-07-04T08:52Z
OSIRIS-APEX = 2026-07-04T01:03Z
Parker Solar Probe = 2026-07-02T05:12Z
STEREO A = 2026-07-03T06:00Z
2: Result 2 (5.5 AU)
Earth = 2026-07-03T03:34Z
BepiColombo = 2026-07-01T21:13Z
Europa Clipper = 2026-07-04T21:01Z
Juice = 2026-07-04T08:01Z
OSIRIS-APEX = 2026-07-04T00:43Z
Parker Solar Probe = 2026-07-02T04:56Z
STEREO A = 2026-07-03T06:00Z
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2026-06-30T23:06Z |
Tony Iampietro on 2026-06-30T23:21Z |
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CME Analysis
|
M2M_CATALOG |
SH
|
true |
SWPC_CAT |
-3.0 |
-1.0 |
1236.0 |
O |
42.0 |
2026-06-30T23:23Z |
Preliminary shock analysis with only several available GOES CCOR-1 frames. Due to the limited frames and full halo presentation, the shock width could vary, impacting speed. Current preliminary analysis of the shock is consistently around 1200 km/s, with high confidence in the latitude and longitude. |
1: Result 1 (2.0 AU)
Earth = 2026-07-02T18:24Z
BepiColombo = 2026-07-01T16:16Z
Europa Clipper = 2026-07-04T02:42Z
Juice = 2026-07-03T22:13Z
OSIRIS-APEX = 2026-07-03T12:02Z
Parker Solar Probe = 2026-07-01T23:43Z
STEREO A = 2026-07-03T04:00Z
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2026-06-30T23:18Z |
Tony Iampietro on 2026-06-30T23:21Z |
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