DONKI Header

Space Weather Database Of Notifications, Knowledge, Information (DONKI)

DONKI: Menu Page

Go to:

DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2024-06-08T01:53Z ( STEREO A: SECCHI/COR2 )
All Detecting Spacecrafts:
STEREO A: SECCHI/COR2
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-06-08T01:53:00-CME-001 (version 1)
Source Location: S17W68
Active Region Number: 13697
Note Keyword:
FOV: Front Bright front; may be evidence of pileup
HAL: Halo CME
SEP: Solar Energetic Particle event
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
FIL: Filament eruption
OFL: Moving/Opening field lines
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
FS: Flux Rope and Shock Candidate
L: Loop
Note: Large halo CME visible in STEREO A COR2 and SOHO LASCO C2 and C3 imagery. The source appears to be two back-to-back M-class flares from AR13697 with associated dimming signature to the north as well as nice filament ejecta to the west and north. Post-eruptive arcades are beginning to show in SDO/AIA 193. There is a large EUV wave associated with this event, as best seen in SDO/AIA 211.

Submitted on 2024-06-08T03:59Z by Carina Alden

A Notification with ID 20240608-AL-010 was sent on 2024-06-08T04:43Z

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 M2M_CATALOG LE true SWPC_CAT 44.0 -10.0 1106.0 O 45.0 2024-06-08T04:59Z BULK measurement made with more complete SOHO frames in LASCO C2/C3 following its downlink backfill. Very little has changed between the preliminary analysis, finding a good triangulation between SOHO and STEREO coronagraphs here. 1: Result 1 (2.0 AU)
Earth = 2024-06-10T14:35Z (PE: -2.0 h)
Lucy = 2024-06-12T20:15Z
Parker Solar Probe = 2024-06-09T07:38Z
STEREO A = 2024-06-10T04:45Z (PE: 1.7 h)
Mars = 2024-06-11T17:00Z
OSIRIS-APEX = 2024-06-10T21:00Z
Tony Iampietro on 2024-06-08T19:09Z
CME Analysis M2M_CATALOG SH true SWPC_CAT 24.0 -3.0 1528.0 O 45.0 2024-06-08T03:59Z SHOCK measurement made with more complete SOHO frames in LASCO C2/C3 following its downlink backfill. This shock front is dimpled between two apparent fronts, seen in both SOHO and STEREO coronagraphs, which made for some difficulty triangulating the two images. Eventually settled on a triangulation using the top of the halo shock as the shared feature between both, finding a good fit. 1: Result 1 (2.0 AU)
Earth = 2024-06-09T22:07Z (PE: -18.5 h)
Lucy = 2024-06-11T17:36Z
Parker Solar Probe = 2024-06-09T14:02Z
STEREO A = 2024-06-09T17:22Z (PE: -9.7 h)
Mars = 2024-06-12T11:00Z
Tony Iampietro on 2024-06-08T19:09Z
CME Analysis M2M_CATALOG LE false SWPC_CAT 43.0 -10.0 1126.0 O 45.0 2024-06-08T04:50Z PRELIMINARY ANALYSIS. SOHO imagery is currently downlinking, preventing from further triangulation. This analysis is based on the BULK of the CME. 1: Result 1 (2.0 AU)
Earth = 2024-06-10T14:31Z (PE: -2.1 h)
Lucy = 2024-06-12T20:49Z
Parker Solar Probe = 2024-06-09T06:57Z
STEREO A = 2024-06-10T04:16Z (PE: 1.2 h)
Mars = 2024-06-11T16:30Z
OSIRIS-APEX = 2024-06-10T20:00Z
Carina Alden on 2024-06-08T04:30Z
CME Analysis M2M_CATALOG SH false SWPC_CAT 24.0 -2.0 1376.0 O 45.0 2024-06-08T03:56Z PRELIMINARY ANALYSIS of the SHOCK front of the CME. 1: Result 1 (2.0 AU)
Earth = 2024-06-09T23:19Z (PE: -17.3 h)
Lucy = 2024-06-11T17:50Z
Parker Solar Probe = 2024-06-09T13:22Z
STEREO A = 2024-06-09T18:15Z (PE: -8.8 h)
Mars = 2024-06-12T08:00Z
Tony Iampietro on 2024-06-08T17:31Z



All directly linked activities:
2024-06-08T00:39:00-FLR-001
FLR Type: M3.3
2024-06-08T01:23:00-FLR-001
FLR Type: M9.7
2024-06-08T02:25:00-SEP-001
GOES-P: SEISS >100 MeV
2024-06-08T02:55:00-SEP-001
GOES-P: SEISS >10 MeV
2024-06-08T03:09:00-SEP-001
MODEL: REleASE:ACE/EPAM 28.2-50.1 MeV
2024-06-08T03:34:00-SEP-001
SOHO: COSTEP 28.2-50.1 MeV
2024-06-08T03:36:00-SEP-001
SOHO: COSTEP 15.8-39.8 MeV
2024-06-08T04:14:00-SEP-001
STEREO A: IMPACT 13-100 MeV
2024-06-08T04:14:00-SEP-002
MODEL: REleASE:ACE/EPAM 15.8-39.8 MeV
2024-06-08T04:20:00-SEP-001
MODEL: REleASE:SOHO/EPHIN 15.8-39.8 MeV
2024-06-08T04:48:00-SEP-001
MODEL: REleASE:SOHO/EPHIN 28.2-50.1 MeV
2024-06-10T03:04:00-IPS-001
Location: STEREO A
2024-06-10T16:36:00-IPS-001
Location: Earth


Comments by users:
0 comment received.
Insert title here

The Moon to Mars Space Weather Analysis Office and other entities provide data to DONKI as a courtesy to the community.
By visiting this site, you acknowledge that you understand and agree to the Important Disclaimer Notice

If you are looking for the official U.S. Government forecast for space weather, please go to NOAA's Space Weather Prediction Center (https://swpc.noaa.gov). This "Experimental Research Information" consists of preliminary NASA research products and should be interpreted and used accordingly.

Curator: Chiu Wiegand | NASA Official: Dr. Masha Kuznetsova | Privacy and Security Notices | Accessibility | CCMC Data Policy