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In this paper, we analyze time series measurements of PSR B0943+10 and fitthem with a non-radial oscillation model. The model we apply was firstdeveloped for total intensity measurements in an earlier paper, and expanded toencompass linear polarization in a companion paper to this one. We use PSRB0943+10 for the initial tests of our model because it has a simple geometry,it has been exhaustively studied in the literature, and its behavior iswell-documented. As prelude to quantitative fitting, we have reanalyzedpreviously published archival data of PSR B0943+10 and uncovered subtle butsignificant behavior that is difficult to explain in the framework of thedrifting spark model. Our fits of a non-radial oscillation model are able tosuccessfully reproduce the observed behavior in this pulsar.

A Quantitative Non-radial Oscillation Model for the Subpulses in PSR B0943+10