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A comparative analysis of Washington color-magnitude diagrams (CMDs) for 14star clusters and respective surrounding fields in the Large Magellanic Cloud(LMC) outer disk is presented. Each CCD frame including field and respectivecluster covers an area of 185 arcmin^2. The stellar population sampled is ofintermediate age and metallicity. CMD radial analysis involving star countratios, morphology and integrated light properties are carried out. Luminosityfunctions (LFs) are also presented. Two main results are: (i) Within the range4<R(kpc)<8, the distance from the LMC center is well correlated with theaverage age in the sense that inner fields are younger and; (ii) Beyondapproximately 8kpc the outer fields do not show evidence of a significantintermediate-age component in their stellar populations, as inferred from redgiant clump star counts.Comment: 27 pages, 4 tables, 11 figures; accepted by the A

Statistics of Stellar Populations of Star Clusters and Surrounding Fields in the Outer Disk of the Large Magellanic Cloud