Low temperature emission measurements were performed at atmospheric and hig
h pressures in KZnF3:Co2+. Comparing the zero-phonon line positions and usi
ng the phonon dispersion relation of the host material, the fine structure
in the emission spectrum was identified. Pressure coefficients were obtaine
d for several among the emission lines from which the values for zero-phono
n lines were deduced. Analysis shows that the spin-orbit parameter changes
with pressure are negligible in this material. (C) 1999 American Institute
of Physics. [S0021-9606(99)70608-2].