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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2016-07-28T22:24Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2016-07-28T22:24:00-CME-001 (version 2)
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: The source of this CME is a filament eruption seen close to disk center in AIA 193/304 starting ~18:00 (with an activation/slow rise phase starting several hours earlier). AIA 304 shows the lift-off of the absorption structure, AIA 193 shows extended brightenings along the filament channel from about ~E20 to W40 in longitude. This eruption produced a faint halo in STA and C2/3.
Submitted on 2016-07-29T18:04Z by Karin
Muglach
A Notification with ID
20160729-AL-001 was sent on 2016-07-29T16:53Z
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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
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M2M_CATALOG |
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true |
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10.0 |
7.0 |
350.0 |
S |
45.0 |
2016-07-29T08:50Z |
The CME is a very faint halo in all 3 coronagraphs (STA, C2/3). Longitude can be about +-10 (around the one used in the model), speed can vary from 200-400 km/s, 350 km/s was at the higher end of possible speeds. |
1: Result 1 (2.0 AU)
Earth = 2016-08-01T12:00Z
(PE: -16.3 h)
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Karin Muglach on 2016-07-29T18:07Z |
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