Finding datasets specifically for solar cosmic rays can be challenging, as most cosmic rays originate from outside the solar system, with the sun contributing minimally. Key sources of cosmic rays include active galactic cores, supernovae, gamma-ray bursts, and quasars. To differentiate solar particles from galactic cosmic radiation, researchers typically analyze specific characteristics of the particles. Useful resources for solar particle data include NOAA's GOES proton flux and NASA's various cosmic ray monitoring sites. Accessing these datasets can provide valuable insights into solar cosmic ray activity.