The Ulysses Catalog of Solar Hard X-Ray Flares is a comprehensive, 13-year dataset (1990–2003+) from the Solar X-ray/Cosmic Gamma-Ray Burst (GRB) instrument, covering solar flares with 15-150 keV hard X-ray spectra. Due to its unique, out-of-ecliptic orbit, the instrument provided stereoscopic observations of flares, including those hidden from Earth-orbiting satellites, allowing analysis of "thermal feed-through" and coronal components.
See publication DOI 10.1007/s11207-009-9387-9
Version:2.7.1
Version:2.7.1
The Ulysses Catalog of Solar Hard X-Ray Flares is a comprehensive, 13-year dataset (1990–2003+) from the Solar X-ray/Cosmic Gamma-Ray Burst (GRB) instrument, covering solar flares with 15-150 keV hard X-ray spectra. Due to its unique, out-of-ecliptic orbit, the instrument provided stereoscopic observations of flares, including those hidden from Earth-orbiting satellites, allowing analysis of "thermal feed-through" and coronal components.
See publication DOI 10.1007/s11207-009-9387-9
| Role | Person | StartDate | StopDate | Note | |
|---|---|---|---|---|---|
| 1. | Author | spase://SMWG/Person/Cecil.Tranquille | |||
| 2. | Author | spase://SMWG/Person/Kevin.C.Hurley | |||
| 3. | MetadataContact | spase://SMWG/Person/Olga.Y.Uritskaya |
Column indicates whether the flare is seen as a count rate increase in the Ulysses data (Y) or not (N), or whether it is not known (?) due to
missing telemetry or to a high background caused by in situ charged particles.
Flare – Sun – Ulysses (F – S – U) angle in degrees
The column provides the peak count rate (non-normalized and corrected for rollover and dead time effects where necessary) measured by GRB during the event if seen.