Preliminary analysis of observed kinematic fields from RiVorS reveals the presence of a number of pronounced, small-scale convergence signatures with varying thermodynamic characteristics. This work utilizes linear, least-squares derivative (LLSD) analysis to produce rotational and divergent shear fields for available WSR-88D and mobile radar data collected during the project. These fields are used to examine storm structure in the low and near-ground levels and attempt to infer processes that may yield notable near-surface kinematic features encountered during RiVorS deployments. Quality-controlled mobile mesonet measurements are matched in space and time to radar-derived fields to explore the evolution of these features and their parent storms. Finally, observed characteristics of RiVorS storms are compared to those of other well-sampled supercells and evaluated within the context of existing conceptual models with a focus on the development of significant low-level rotation.