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: 2024-07-05T19:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2024-07-05T19:24:00-CME-001 (version 1)
Note Keyword:
DFL: Likely deflection of the event within the FOV
OVR: Event partially overlaps with another CME
Source Signature Keyword:
OFL: Moving/Opening field lines
Morphology Keyword:
L: Loop
Note: CME visible to the SW in SOHO LASCO C2/C3 and STEREO-A COR2. Source is opening field lines on the SW limb, most likely from Active Region 13724 which was at about S15W110 at the time of the eruption, as seen in SDO AIA 171/193 starting at 2024-07-05T18:57Z. There is also some movement/activity centered at S05W50 on the disk at a similar time, but the movement more likely to be associated with this eruption seems to be from the SW limb.

Submitted on 2024-07-06T16:20Z by Hannah Hermann

A Notification with ID 20240706-AL-001 was sent on 2024-07-06T18:19Z
A Notification with ID 20240707-AL-001 was sent on 2024-07-07T14:22Z

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 110.0 -32.0 633.0 C 31.0 2024-07-06T00:42Z Measurement taken using best fit between coronagraphs and approximate source location based on UV imagery of the Earth-facing disk. 1: Result 1 (2.0 AU)
OSIRIS-APEX = 2024-07-08T08:00Z
Mars = 2024-07-11T04:00Z
2: Result 2 (2.0 AU)
OSIRIS-APEX = 2024-07-08T08:00Z
Mars = 2024-07-11T00:00Z
STEREO A = 2024-07-09T08:00Z
3: Result 3 (2.0 AU)
Mars = 2024-07-11T11:18Z
OSIRIS-APEX = 2024-07-08T06:36Z
Solar Orbiter = 2024-07-09T04:00Z
STEREO A = 2024-07-09T06:00Z
Hannah Hermann on 2024-07-06T16:21Z



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