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We present phase-resolved spectroscopy, photometry and circularspectropolarimetry of the eclipsing polar UZ Fornacis. Doppler tomography ofthe strongest emission lines using the inside-out projection revealed thepresence of three emission regions: from the irradiated face of the secondarystar, the ballistic stream and the threading region, and the magneticallyconfined accretion stream. The total intensity spectrum shows broad emissionfeatures and a continuum that rises in the blue. The circularly polarizedspectrum shows the presence of three cyclotron emission harmonics at $\sim$4500\AA{}, 6000 \AA{} and 7700 \AA{}, corresponding to harmonic numbers 4, 3, and2, respectively. These features are dominant before the eclipse and disappearafter the eclipse. The harmonics are consistent with a magnetic field strengthof $\sim$57 MG. We also present phase-resolved circular and linearphotopolarimetry to complement the spectropolarimetry around the times ofeclipse. MeerKAT radio observations show a faint source which has a peak fluxdensity of 30.7 $\pm$ 5.4 $\mu$Jy/beam at 1.28 GHz at the position of UZ For.

A spectroscopic, photometric, polarimetric and radio study of the eclipsing polar UZ Fornacis: the first simultaneous SALT and MeerKAT observations