The micromaser possesses a variety of dynamical phase transitions para
metrized by the flux of atoms and the time of flight of the atom withi
n the cavity. We discuss how these phases may be revealed to an observ
er outside the cavity using the long-time correlation length in the at
omic beam. Some of the phase transitions are not reflected in the aver
age excitation level of the outgoing atom, which is the commonly used
observable. The correlation length is directly related to the leading
eigenvalue of the time evolution operator, which we study in order to
elucidate the phase structure. We find that as a function of the time
of flight the transition from the thermal to the maser phase is charac
terized by a sharp peak in the correlation length. For longer times of
flight there is a transition to a phase where the correlation length
grows exponentially with the flux. We present a detailed numerical and
analytical treatment of the different phases and discuss the physics
behind them.