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
Version:2.6.1
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
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | HostContact | spase://SMWG/Person/Nariaki.V.Nitta |
Links to documentation, images, movies, software and contact information.
STEREO/EUVI event Catalogue Number.
Observation date
Start time
End time
Carrington longitude of active region
Instrument cadence.
A=Ahead only without Behind data
B=Behind only without Ahead data
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.
Peak RHESSI energy range in which event is observed.
Counts in peak RHESSI energy range.
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
CME reported by one or both of the following: L=LASCO/SOHO S=SECCHI/Cor-1,Cor-2