Small-scale coherent magnetic structures in the solar wind have drawn considerable interest in recent years. Some of the outstanding questions include 1) their origin (do they originate from the solar corona or are they generated locally via turbulent cascade?), and 2) their role in solar wind heating and particle energization. Parker Solar Probe and Solar Orbiter observations have shown that some small local energization events (the exact sources are unclear) are not easily explained by traditional acceleration mechanisms such as solar flares and shocks, especially close to the Sun. Turbulent reconnection and stochastic acceleration due to coherent magnetic structures are possible explanations. In this session, we solicit contributions addressing but not limited to the observational analysis of coherent magnetic structures, the related analysis of solar wind heating and particle energization. Theories and modeling that focus on local particle energization mechanisms are also welcome.