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: 2023-08-05T07:12Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-08-05T07:12:00-CME-001 (version 1)
Source Location: S10W68
Note Keyword:
3P: 3-part structure CME
PRM: Prominence material (filamentary structures)
SEP: Solar Energetic Particle event
Source Signature Keyword:
FIL: Filament eruption
Morphology Keyword:
F: Flux Rope
FS: Flux Rope and Shock Candidate
Note: Wide CME seen to the south and west in SOHO and STEREO A associated with a long duration M1.6-class solar flare and erupting filament occurring near S10W68. The faint shock presents a full halo with preference towards the west. The event was not captured in SDO EUV imagery due to an ongoing eclipse, however, GOES SUVI detected the event. Around 2023-08-05T06:45Z, a dark filament near the western portion of the disk is seen lifting off, becoming a bright structure as it leaves the disk towards the west.
Submitted on 2023-08-05T13:57Z by Chris Stubenrauch

A Notification with ID 20230805-AL-007 was sent on 2023-08-05T14:43Z

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, earlier measurements are marked as false when new or more accurate measurements are made. This is a helpful flag if you would like to download only one most accurate CME analysis per CME
 Technique Long Lat Speed Type Half Width Time 21.5 Note WSA-ENLIL+Cone Result(s) Submitted By
CME Analysis M2M_CATALOG COR true SWPC_CAT 63.0 -17.0 1044.0 O 46.0 2023-08-05T10:28Z Measurement of the brightest feature/bulk of the CME using two spacecraft. 1: Result 1 (2.0 AU)
Earth = 2023-08-07T23:00Z (PE: 11.9 h)
OSIRIS-REx = 2023-08-08T21:00Z
Parker Solar Probe = 2023-08-07T11:00Z
Chris Stubenrauch on 2023-08-05T13:58Z



All directly linked activities:
2023-08-05T06:18:00-FLR-001
FLR Type: M1.6
2023-08-05T10:00:00-SEP-001
STEREO A: IMPACT 13-100 MeV
2023-08-05T10:19:00-SEP-001
SOHO: COSTEP 15.8-39.8 MeV
2023-08-05T10:47:00-SEP-001
SOHO: COSTEP 28.2-50.1 MeV
2023-08-05T10:59:00-SEP-001
MODEL: REleASE:ACE/EPAM 15.8-39.8 MeV
2023-08-05T11:15:00-SEP-001
GOES-P: SEISS >10 MeV
2023-08-05T12:33:00-SEP-001
MODEL: REleASE:SOHO/EPHIN 15.8-39.8 MeV
2023-08-07T08:46:00-IPS-001
Location: STEREO A
2023-08-07T11:07:00-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 Collection Consent Agreement