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STEREO/EUVI Event Catalog (>C1 GOES class or >12 keV RHESSI)

ResourceID
spase://NASA/Catalog/STEREO/SECCHI/EUVI/EventCatalog

Description
This is a catalogue of flare/CME events observed with EUVI when the spacecraft separation angle is small to moderate when classical stereoscopy is feasible. The list contains also the peak fluxes in soft X rays and hard X rays. EUVI Classification: A=Ahead only without Behind data B=Behind only without Ahead data I=Impulsive time profile (peak in coincidence with SXR) P=Postflare loop or arcade (delayed emission after SXR peak) D=Dimming (EUV flux decreases after SXR peak) E=Eruptive filament O=Occulted for A (if flare position is east) or B (if west) T=Test images (or poor image quality) W=Waves and oscillations CME reported: L=LASCO/SOHO, S=SECCHI/Cor-1,Cor-2

Metadata Rights
CC0-1.0: Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions. The actual data/software may be subject to a different license.

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Details

Version:2.7.1

Catalog

ResourceID
spase://NASA/Catalog/STEREO/SECCHI/EUVI/EventCatalog
NamingAuthority
NASA
ResourceType
Catalog
ResourceHeader
ResourceName
STEREO/EUVI Event Catalog (>C1 GOES class or >12 keV RHESSI)
ReleaseDate
2026-02-02 13:10:26Z
RevisionHistory
RevisionEvent
ReleaseDate
2024-08-20 10:02:14
Note
Only known prior ReleaseDate of the metadata
RevisionEvent
ReleaseDate
2026-02-02 13:10:26Z
Note
Added MetadataRightsList. Added ResourceType and NamingAuthority. Updated to 2.7.1. Changed http to https in top-level schemaLocation attribute. Fixed version number separator in top-level schemaLocation attribute. ZCB
Description
This is a catalogue of flare/CME events observed with EUVI when the spacecraft separation angle is small to moderate when classical stereoscopy is feasible. The list contains also the peak fluxes in soft X rays and hard X rays. EUVI Classification: A=Ahead only without Behind data B=Behind only without Ahead data I=Impulsive time profile (peak in coincidence with SXR) P=Postflare loop or arcade (delayed emission after SXR peak) D=Dimming (EUV flux decreases after SXR peak) E=Eruptive filament O=Occulted for A (if flare position is east) or B (if west) T=Test images (or poor image quality) W=Waves and oscillations CME reported: L=LASCO/SOHO, S=SECCHI/Cor-1,Cor-2
Contacts
Role Person StartDate StopDate Note
1. HostContact spase://SMWG/Person/Nariaki.V.Nitta
InformationURL
Name
STEREO - SECCHI - EUVI (LMSAL)
URL
Description
Links to documentation, images, movies, software and contact information.
AccessInformation
RepositoryID
AccessURL
Name
Early EUVI Event Catalog [195 events] at LMSAL
URL
Format
Text
InstrumentIDs
PhenomenonType
CoronalMassEjection
PhenomenonType
SolarFlare
TimeSpan
StartDate
2006-12-04 17:00:00
StopDate
2009-07-08 06:00:00
Parameter #1
Name
#
Description
STEREO/EUVI event Catalogue Number.
Support
SupportQuantity
Other
Parameter #2
Name
DATE
Description
Observation date
Support
SupportQuantity
Temporal
Parameter #3
Name
START
Description
Start time
Support
SupportQuantity
Temporal
Parameter #4
Name
END
Description
End time
Support
SupportQuantity
Temporal
Parameter #5
Name
POSITION
Description
Carrington longitude of active region
Support
SupportQuantity
Positional
Parameter #6
Name
CAD
Description
Instrument cadence.
Support
SupportQuantity
Other
Parameter #7
Name
SC
Description
A=Ahead only without Behind data B=Behind only without Ahead data
Support
SupportQuantity
Other
Parameter #8
Name
GOES
Description
Importance of flare at X-ray wavelengths -- the peak flux measured at Earth in the 0.1 to 0.8 nm range in units of W m-2.
Support
SupportQuantity
Other
Parameter #9
Name
RHESSI
Description
Peak RHESSI energy range in which event is observed.
Support
SupportQuantity
Other
Parameter #10
Name
CTS
Description
Counts in peak RHESSI energy range.
Support
SupportQuantity
Other
Parameter #11
Name
COMMENTS
Description
Comments using the following EUVI Classification: A=Ahead only without Behind data B=Behind only without Ahead data I=Impulsive time profile (peak in coincidence with SXR) P=Postflare loop or arcade (delayed emission after SXR peak) D=Dimming (EUV flux decreases after SXR peak) E=Eruptive filament O=Occulted for A (if flare position is east) or B (if west) T=Test images (or poor image quality) W=Waves and oscillations
Support
SupportQuantity
Other
Parameter #12
Name
CME
Description
CME reported by one or both of the following: L=LASCO/SOHO S=SECCHI/Cor-1,Cor-2
Support
SupportQuantity
Other