Ultrahigh energy gamma rays produce electron-positron pairs in interac
tions on the geomagnetic field. The pair electrons suffer magnetic bre
msstrahlung and the energy of the primary gamma ray is shared by a bun
ch bf lower energy secondaries. These processes reflect the structure
of the geomagnetic field and cause experimentally observable effects.
The study of these effects with future giant air shower arrays dan ide
ntify the nature of the highest energy cosmic rays as either gamma ray
s or nuclei.