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: 2023-12-15T07:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2023-12-15T07:48:00-CME-001 (version 1)
Source Location: N03W65
Active Region Number: 13514
Note Keyword:
Source Signature Keyword:
FLR: Flare
PEA: Post eruption arcade
OFL: Moving/Opening field lines
BR: Brightening
DIM: Dimming
EUVW: EUV Wave
Morphology Keyword:
LS: Loop and Shock Candidate
Note: CME seen to the SW in SOHO LASCO C2/C3 and STEREO A COR2. This CME is associated with two M-class flares from Active Region 13514. An EUV wave is seen in SDO AIA 171/193, propagating southward, generally down the W60 longitude line, starting at 2023-12-15T07:21Z. Brightening and some ejecta seen in SDO AIA 304.
Submitted on 2023-12-15T14:38Z by Hannah Hermann

A Notification with ID 20231215-AL-009 was sent on 2023-12-15T18:36Z

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 LE true SWPC_CAT 60.0 -22.0 1101.0 O 37.0 2023-12-15T11:04Z Bulk measurement made using source location and best fit between coronagraphs. Southern deflection from source location is likely associated with the southern direction of EUV wave propagation as seen in UV imagery. 1: Result 1 (2.0 AU)
OSIRIS-APEX = 2023-12-16T10:44Z
STEREO A = 2023-12-18T07:00Z
2: Result 2 (5.5 AU)
OSIRIS-APEX = 2023-12-16T10:46Z
Hannah Hermann on 2023-12-15T17:15Z
CME Analysis M2M_CATALOG SH false SWPC_CAT 60.0 -26.0 1264.0 O 39.0 2023-12-15T10:40Z Shock measurement made using source location and best fit between coronagraphs. Deflection from source location is likely associated with the direction of EUV wave propagation as seen in UV imagery. 1: Result 1 (2.0 AU)
OSIRIS-APEX = 2023-12-16T08:45Z
Hannah Hermann on 2023-12-15T14:40Z



All directly linked activities:
2023-12-15T07:03:00-FLR-001
FLR Type: M6.3
2023-12-15T07:23:00-FLR-001
FLR Type: M6.9
2023-12-15T10:05:00-SEP-001
MODEL: REleASE:ACE/EPAM 15.8-39.8 MeV
2023-12-15T14:57:00-SEP-001
MODEL: REleASE:SOHO/EPHIN 15.8-39.8 MeV
2023-12-15T15:42:00-SEP-001
SOHO: COSTEP 15.8-39.8 MeV
2023-12-15T23:45:00-SEP-001
GOES-P: SEISS >10 MeV


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