The analytical expression for the angular integral flux of atmospheric muon
s in matter with an explicit relation of its parameters with those of the s
ea level spectrum is obtained, The fitting formula for the sea level muon s
pectrum at different zenith angles for a spherical atmosphere is proposed.
The concrete calculations for pure water are presented. Fluctuations of muo
n energy losses are taken into account by means of a parametrized correctio
n factor calculated using survival probabilities resulting from Monte Carlo
simulations. Parametrizations of all continuous energy losses are obtained
using the most recent expressions for muon inter action cross sections. Th
e corresponding parametrization errors and field of method application are
comprehensively discussed. The proposed formulas could be useful primarily
for experimentalists processing data of arrays located deep under water or
ice.