  Large spherical scintillation detectors are playing an increasingly important
role in experimental neutrino physics studies. From the instrumental point of
view the primary signal response of these set-ups is constituted by the time
and amplitude of the anode pulses delivered by each individual phototube
following a particle interaction in the scintillator. In this work, under some
approximate assumptions, we derive a number of analytical formulas able to give
a fairly accurate description of the most important timing features of these
detectors, intended to complement the more complete Monte Carlo studies
normally used for a full modelling approach. The paper is completed with a
mathematical description of the event position distributions which can be
inferred, through some inference algorithm, starting from the primary time
measures of the photomultiplier tubes.
