  In this paper we review the Myrzakulov Gravity models (MG-N, with $\mathrm{N
= I, II, \ldots, VIII}$) and derive their respective metric-affine
generalizations (MAMG-N), discussing also their particular sub-cases. The field
equations of the theories are obtained by regarding the metric tensor and the
general affine connection as independent variables. We then focus on the case
in which the function characterizing the aforementioned metric-affine models is
linear and consider a Friedmann-Lema\^{i}tre-Robertson-Walker background to
study cosmological aspects and applications.
