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There are either a near kinematic distance of 5.5 kpc or a far distance of8.8 kpc for a Galactic supernova remnant (SNR) G32.8$-$0.1 derived by using therotation curve of the Galaxy. Here we make sure that the remnant distance isthe farther one 8.8 kpc through solving a group of equations for the shell-typeremnants separately at the adiabatic-phase and the radiative-phase. For SNRG346.6$-$0.2 we determine its distance also the farther one 11 kpc rather thanthe nearer one 5.5 kpc.

Distances to Two Galactic Supernova Remnants: G32.8-0.1 and G346.6-0.2