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We report the first observations of far-ultraviolet (FUV: 1000 -- 1150 \AA)diffuse radiation from the Small Magellanic Cloud (SMC) using observations fromthe {\em Far Ultraviolet Spectroscopic Explorer (FUSE)}. The strength of FUVdiffuse surface brightness in the SMC ranges from the detection limit of 2000photons cm$^{-2}$ s$^{-1}$ sr$^{-1}$ \AA$^{-1}$ to a maximum of $3 \times10^{5}$ photons cm$^{-2}$ s$^{-1}$ sr$^{-1}$ \AA$^{-1}$ at 1004 \AA. Thecontribution of diffuse emission to the total radiation field was found to be34% at 1004 \AA to 44% at 1117 \AA with a maximum observed uncertainty of 30%.There is a striking difference between the FUV diffuse fraction from the SMCand the Large Magellanic Cloud (LMC) with the SMC fraction being higherprobable because the higher dust albedo. The FUV diffuse emission correlateswith H$\alpha$ emission in the H {\small II} regions of the SMC.

Observations of Far-Ultraviolet Diffuse Emission from the Small Magellanic Cloud