Found 8 datasets matching filters.
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Time-dependent detector response matrices for each GBM detector covering the duration of every GBM flare. Needed in the spectral analysis software to relate observed count-rate spectra to model...
Search relevance: 1.00 | Views last month: 2 | Published on: 2025-10-06 -
Time histories of NaI, GBO, and GOES data, with flare and day/night markers. Orbital plots are on RHESSI orbit times.
Search relevance: 1.00 | Views last month: 1 | Published on: 2025-08-04 -
LAT solar gamma-ray flux > 100 MeV, one point per solar exposure (i.e. average of the 20-40 minutes of solar observation every ~1.5 hours) calculated by two different methods.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
Time histories of NaI, GBO, and GOES data, with flare and day/night markers. Orbital plots are on RHESSI orbit times.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-10-20 -
LAT data between 100 MeV and 10 GeV filtered for solar counts in 1-minute time bins, no energy binning, using light-bucket method. Contains exposure (cm^2 s) information.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
LAT solar gamma-ray flux > 100 MeV, one point per solar exposure (i.e. average of the 20-40 minutes of solar observation every ~1.5 hours) calculated by two different methods.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04 -
LAT solar gamma-ray flux > 100 MeV, one point per solar exposure (i.e. average of the 20-40 minutes of solar observation every ~1.5 hours) calculated by two different methods.
Search relevance: 1.00 | Views last month: 0 | Published on: 2026-03-07 -
Time histories of NaI, GBO, and GOES data, with flare and day/night markers. Orbital plots are on RHESSI orbit times.
Search relevance: 1.00 | Views last month: 0 | Published on: 2025-08-04
