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Global Aerosol Optical Depths and Longitudinal Shower Development in Solid Proton and Gamma Ray Distributions

Study of Solid Protons and Gamma Rays in near-equatorial orbit, evaluating Magnetic Bremsstrahlung vs. LPM Effect, with focus on Aerosol Optical Depths and Shower Development. Data from HiRes Stereo Events analyzed for varying Aerosol Heights.

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Global Aerosol Optical Depths and Longitudinal Shower Development in Solid Proton and Gamma Ray Distributions

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  1. UHE Xmax Distributions Solid: Protons Dashed: Gamma Rays dominated by magnetic bremsstrahlung (arriving from east/west for near equatorial orbit) Dotted: Gamma Rays dominated by LPM effect (arriving from north/south for near equatorial orbit)

  2. LPM Effect and Longitudinal Shower Development

  3. Global Aerosol Optical Depths

  4. HiRes Stereo Event lAerosol = 22.5 km lAerosol = 12.5 km

  5. HiRes Stereo Event: lAero = 25.0 km

  6. HiRes Stereo Event: lAero = 22.5 km

  7. HiRes Stereo Event: lAero = 12.5 km

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