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: 2024-03-15T17:36Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-03-15T17:36:00-CME-001 (version 1)
Source Location: S40E60
Note Keyword:
Source Signature Keyword:
OFL: Moving/Opening field lines
DIM: Dimming
Morphology Keyword:
L: Loop
Note: CME to the southeast in SOHO LASCO C2, C3, and STEREO A COR2. Source is the clear liftoff of material seen on the SE limb in SDO AIA 171 starting as early as 2024-03-15T15:30Z. Subtle dimming on the Earth-facing disk, centered at S40E60, can be seen in SDO AIA 193 at 2024-03-15T18:40Z. There is some field line movement seen on GOES SUVI 284 and 195 at the same time and location as this dimming. Small amount of ejecta seen on the SE limb in GOES SUVI 304 at 2024-03-15T18:30Z, which is long after the start time of this CME, however this is a prolonged and relatively slow CME.

Submitted on 2024-03-16T16:02Z by Hannah Hermann

No Notification has been sent for this activity yet.

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 -57.0 -61.0 368.0 S 33.0 2024-03-16T07:19Z Candidate source location on the Earth-facing disk (dimming at S40E60) is very subtle, but using this candidate source location with southward deflection yields a better stereoscopic fit than using a longitude beyond the limb. Only two frames of STEREO A COR2 difference imagery were available for this CME due to a data gap which lasted from 2024-03-15T15:53Z to 2024-03-16T03:23Z in difference imagery. Not modeled Hannah Hermann on 2024-03-16T16:18Z
CME Analysis M2M_CATALOG LE false Plane-of-sky NONE -65.0 334.0 S 34.0 2024-03-16T07:48Z Initial measurement taken using Plane-of-Sky method due to uncertainty of source location. Not modeled Hannah Hermann on 2024-03-16T16:05Z



All directly linked activities:
No Linked Activity Found.


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