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On the base of its high altitude and nearly full coverage, the ARGO-YBJ experiment could play a important role in bridging satellite/balloon-borne and indirect measurement in the energy spectrum measurment. In this work the light component (proton + helium like) of cosmic rays can be selected from the shower lateral information and the energy of the cosmic ray light component will be calculated. Combining the westward displacement of moon shadow position direction using the same set of data, the construction of an energy scaler from air shower experiment is discussed.

ARGO-YBJ absolute energy scale calibration for light primaries in the multi TeV region by using the Moon shadow