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DONKI: View SW Activity
Coronal Mass Ejection
Catalog: M2M_CATALOG
Start Time: 2020-05-28T01:25Z ( SOHO: LASCO/C2 )
All Detecting Spacecrafts:
SOHO: LASCO/C2
SOHO: LASCO/C3
STEREO A: SECCHI/COR2
Activity ID: 2020-05-28T01:25:00-CME-001 (version 1)
Note Keyword:
Source Signature Keyword:
Morphology Keyword:
Note: The source is unclear. The source was originally thought to be an eruption at 2020-05-28T02:25Z from the unnamed AR off the southeastern limb as seen from STA EUVI 195, but the appearance of the CME to the west in C2/C3 and east in Cor2A, along with the timing of the activity in C2 slightly before this eruption, suggests that the source is more likely in the unseen region on the disk that is currently not viewable, with a source longitude determined from the best agreement between spacecraft for the CME measurement.
Submitted on 2020-05-29T00:30Z by Michael
GreklekMcKeon
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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 |
SWPC_CAT |
136.0 |
4.0 |
217.0 |
S |
24.0 |
2020-05-28T18:03Z |
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1: Result 1 (2.0 AU)
Parker Solar Probe = 2020-05-30T02:11Z
OSIRIS-REx = 2020-06-01T16:00Z
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Michael GreklekMcKeon on 2020-05-29T00:31Z |
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