We report the first detection of a TeV gamma-ray flux from the solar disk (6.3\sigma), based on 6.1 years of data from the High Altitude Water Cherenkov (HAWC) observatory. The 0.5--2.6 TeV spectrum is well fit by a power law, dN/dE = A (E/1 \text{ TeV})^{-\gamma}, with $A = (1.6... Show more