Fermi Solar Flare X-Ray and Gamma-Ray Observations

The Fermi Gamma-ray Space Telescope was launched in June 2008 to explore high-energy phenomena in the Universe. This GI program is targeted specifically at Fermi observations of high-energy solar phenomena, primarily solar flares. We provide quicklook products, data archives, and analysis software covering the solar X-ray and gamma-ray observations of both the Gamma-ray Burst Monitor (GBM) and Large Area Telescope (LAT), with the objective of facilitating and encouraging the broad use of Fermi data by the international solar physics community.

Data and Resources

Additional Info

Field Value
Maintainer Kim Tolbert
Last Updated April 23, 2025, 22:40 (UTC)
Created March 31, 2025, 15:07 (UTC)
accessLevel public
accrualPeriodicity irregular
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harvest_source_id 61638e72-b36c-4866-9d28-551a3062f158
harvest_source_title DNG Legacy Data
identifier NASA-0000242
issued 2018-06-25
landingPage https://data.nasa.gov/dataset/fermi-solar-flare-x-ray-and-gamma-ray-observations
modified 2020-01-29
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publisher National Aeronautics and Space Administration
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