Using the KOSMA 3-m telescope we have made observations of the ^12^CO(J=1-0), (J=2-1) and (J=3-2), and the ^13^CO(J=1-0) and (J=2-1) transitions of the high latitude cloud MBM 32. The backend consisted of a Medium Resolution (channel width 167kHz; MRS), or a High Resolution (channel width 38.6kHz; HRS) acousto-optical Spectrometer. The following tables contain properties of clumps derived from the maps, assuming Gaussian clump parameters from the ^12^CO(J=1-0) MRS data (Table 3) ^12^CO(J=1-0) HRS data (Table 4) ^12^CO(J=2-1) MRS data (Table 5) ^13^CO(J=1-0) HRS data (Table 6). We distinguish between different velocity components.