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 February 19, 2025, 02:29 (UTC)
Created February 19, 2025, 02:29 (UTC)
accessLevel public
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identifier NASA-0000242
issued 2018-06-25
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modified 2020-01-29
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