Abstract
The origin of the extreme energy cosmic rays (EECRs) is a mystery in the contemporary astrophysics. The JEM‐EUSO Mission that mainly aims establishing astronomy using such EECRs with very high statistics will also have realistic capability of detecting gamma rays and neutrinos with ∼1020 eV energies. Aboard the International Space Station, the JEM‐EUSO mission also provides a unique platform to detect and study the air showers from extreme energy gamma rays and neutrinos. In the present paper, we discuss a part of results from our study on properties of gamma ray and neutrino induced air showers and the advantage for space‐based observation.
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