We suggest a new approach to the normalisation of neutron monitor response
to galactic cosmic rays. The reference normalisation count rate is the neut
ron monitor response to the model unmodulated flux of galactic cosmic rays.
A comparison of the actually recorded neutron monitor count rate with the
calculated normalisation count rate can provide one with an observationally
obtained true-of-date integral measure of the current level of solar modul
ation of galactic cosmic rays.