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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2014-04-01T17:00Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO B: SECCHI/COR2
Activity ID: 2014-04-01T17:00:00-CME-001 (version 1)
Source Location: S9E15
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: Filament eruption & dimmings on disk in AIA from around 14:30-17:00.
Submitted on 2014-04-02T15:07Z by Barbara
Thompson
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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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-15.0 |
-9.0 |
450.0 |
S |
50.0 |
2014-04-02T00:19Z |
A speed of 325km/sec was obtained based on the cone model reprojection of the plane of sky speed in LASCO C2 & C3, using the filament eruption as the source. However, the simulation used speed = 450 km/sec because Leila said that slow CMEs usually have too late arrivals. |
1: Result 1 (2.0 AU)
Earth = 2014-04-05T04:50Z
Mars = 2014-04-07T13:37Z
2: Result 2 (2.0 AU)
Earth = 2014-04-04T06:07Z
Mars = 2014-04-05T16:09Z
Spitzer = 2014-04-04T02:23Z
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Barbara Thompson on 2014-04-02T15:07Z |
CME Analysis
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M2M_CATALOG |
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false |
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-15.0 |
-9.0 |
325.0 |
S |
50.0 |
2014-04-02T04:24Z |
This was the original speed measured. The speed entered into the simulation was higher because slow CMEs usually arrive later than predicted. |
Not modeled
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Barbara Thompson on 2014-04-15T21:15Z |
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