One way to rigorously define spinor fields on metric manifolds is through the language of associated bundles. Namely, we have a principal bundle $P \overset{\pi}{\longrightarrow} M$ over $\mathrm{Spin}(n)$ (or whatever other signature) that is a $\rho$-equivariant lift of the orthonormal frame bundle $OFM \rightarrow M$ through the map $\phi: P \rightarrow OFM$, where $\rho: \mathrm{Spin}(n) \rightarrow SO(n)$ is the double-cover map. $(P,\phi)$ prescribes the spin structure.
The associated bundle is then constructed with a typical fiber $F$, which is a representation space of $\mathrm{Spin}(n)$, and where the field takes its values. The transformation behavior of the objects is at that point fixed through the left and right actions of the group on these bundles. The fields are then taken as sections of the associated bundle, which can equivalently be expressed as $\mathrm{Spin}(n)$-equivariant functions on the principal bundle.
The part that is unclear to me is how these are related to the usual spinors that we see in physics. In particular:
The general construction doesn't specify the choice of spin structure $(P, \phi)$. Are there any concrete examples for this choice?
To get 'fields' (in the physics sense) defined on $M$ one usually needs a local trivialization of the principal bundle. How would this be provided in practice?
For tangent vectors, for example, the principal bundle is the frame bundle $FM$, and one can induce the trivialization by a chart $(U, x)$ on the base manifold $M$, namely by giving the section $\alpha: U \rightarrow FM,\,\; p \mapsto (\partial / \partial x)_p$, but this doesn't even port over to $OFM$ since $(\partial / \partial x)_p$ are not necessarily orthonormal.