Understand
We present the calculation of the atmospheric neutrino fluxes for the neutrino experiments proposed at INO, South Pole and Pyh\"asalmi.
- Neutrino fluxes have been obtained using ATMNC, a simulation code for cosmic ray in the atmosphere.
- Even using the same primary flux model and the interaction model, the calculated atmospheric neutrino fluxes are different for the different sites due to the geomagnetic field.
- The prediction of these fluxes in the present paper would be quite useful in the experimental analysis.
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