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: 2024-07-21T16:48Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
Activity ID: 2024-07-21T16:48:00-CME-001 (version 2)
Source Location: N15E20
Active Region Number: 13757
Note Keyword:
DFL: Likely deflection of the event within the FOV
GAP: Data gap
HAL: Halo CME
Source Signature Keyword:
FLR: Flare
FIL: Filament eruption
OFL: Moving/Opening field lines
Morphology Keyword:
Note: Halo CME visible in SOHO LASCO C2 and C3 imagery. STEREO A COR2 is in a data gap during this event. The source of this CME appears to be an M1.0 flare from AR13757 (N15E20) peaking at 2024-07-21T16:31Z. Filament ejecta is visible in SDO/AIA 304 and GOES SUVI 304 with significant northward deflection. The bulk of the CME is likely the brighter portion visible in SOHO LASCO C2/C3 difference imagery to the NE. The fainter halo portion is possibly associated with this event, though there is some uncertainty due to a lack of visible dimming to the south of the source location.

Submitted on 2024-07-21T23:46Z by Carina Alden

A Notification with ID 20240721-AL-003 was sent on 2024-07-21T23:20Z

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 -20.0 42.0 719.0 C 46.0 2024-07-21T21:39Z These parameters are based off of the best fit of the suspected BULK of the CME visible to the NE in SOHO LASCO difference imagery. No STEREO A COR2 imagery is available for this CME. 1: Result 1 (2.0 AU)
Earth = 2024-07-24T16:11Z (PE: 20.4 h)
Lucy = 2024-07-25T16:37Z
Parker Solar Probe = 2024-07-23T12:55Z
STEREO A = 2024-07-24T15:00Z (PE: 17.3 h)
Carina Alden on 2024-07-21T22:50Z
CME Analysis M2M_CATALOG SH true SWPC_CAT -5.0 8.0 1224.0 O 43.0 2024-07-21T19:30Z Parameters based on the potential SHOCK feature using SOHO LASCO C2 and C3 difference imagery. There is uncertainty with this analysis due to lack of stereoscopic viewpoints. 1: Result 1 (2.0 AU)
Earth = 2024-07-23T16:36Z (PE: -3.2 h)
Lucy = 2024-07-24T15:27Z
Parker Solar Probe = 2024-07-22T18:52Z
STEREO A = 2024-07-23T13:58Z (PE: -7.7 h)
Carina Alden on 2024-07-21T23:07Z



All directly linked activities:
2024-07-21T16:18:00-FLR-001
FLR Type: M1.0
2024-07-23T19:48:00-IPS-001
Location: Earth
2024-07-23T21:40:00-IPS-001
Location: STEREO A


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