2.7.1 https://spdx.org/licenses/ SPDX CC0-1.0 https://spdx.org/licenses/CC0-1.0.html Creative Commons Zero v1.0 Universal CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions spase://NASA/Catalog/STEREO/SECCHI/EUVI/EventCatalog NASA Catalog STEREO/EUVI Event Catalog (>C1 GOES class or >12 keV RHESSI) 2026-02-02T13:10:26Z 2024-08-20T10:02:14 Only known prior ReleaseDate of the metadata 2026-02-02T13:10:26Z 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 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 spase://SMWG/Person/Nariaki.V.Nitta HostContact STEREO - SECCHI - EUVI (LMSAL) https://secchi.lmsal.com/EUVI/ Links to documentation, images, movies, software and contact information. spase://SMWG/Repository/LMSAL Early EUVI Event Catalog [195 events] at LMSAL https://secchi.lmsal.com/EUVI/euvi_catalog.txt Text spase://NASA/Instrument/STEREO-A/SECCHI/EUVI spase://NASA/Instrument/STEREO-B/SECCHI/EUVI spase://SMWG/Instrument/RHESSI/HESSI spase://SMWG/Instrument/GOES spase://SMWG/Instrument/SOHO/LASCO CoronalMassEjection SolarFlare 2006-12-04T17:00:00 2009-07-08T06:00:00 # STEREO/EUVI event Catalogue Number. Other DATE Observation date Temporal START Start time Temporal END End time Temporal POSITION Carrington longitude of active region Positional CAD Instrument cadence. Other SC A=Ahead only without Behind data B=Behind only without Ahead data Other GOES 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. Other RHESSI Peak RHESSI energy range in which event is observed. Other CTS Counts in peak RHESSI energy range. Other COMMENTS 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 Other CME CME reported by one or both of the following: L=LASCO/SOHO S=SECCHI/Cor-1,Cor-2 Other