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We report the results of the first 5~GHz southern hemisphere VLBI observations with SHEVE (Southern Hemisphere VLBI Experiment) network (plus Shanghai) performed during a 50 hour period in November 1992. A sample of 23 extragalactic radio sources were observed. Images of 20 sources and structural information on 2 others (1548+056 and 1814$-$637) were obtained. Of the 20 sources, fifteen showed core$-$jet structure (0048$-$097, 0106+013, 0235+164, 0420$-$014, 0458$-$020, 1104$-$445, 1334$-$127, 1504$-$166, 1730$-$130, 1741$-$038, 1921$-$293, 2134+004, 2145+067, 2223$-$052, and 2345$-$167), one had a two$-$sided jet (1510$-$089) and 4 were unresolved at the level of $\sim$0.6~mas (0104$-$408, 1144$-$379, 1519$-$273 and 2216$-$038). There were no compact doubles. Eleven of the 16 core$-$jet (including the two$-$sided jet) sources showed evidence of bent jets. We also found evidence, based on the temporal variability of radio flux density and previous images, for superluminal motion in 4 sources: 0106+013(8.2c), 0420$-$014(3.9c), 1334$-$127(4.5c) and 2345$-$167(5.0c).