  We perform direct numerical simulations of quasi-static magnetohydrodynamic
turbulence, and compute various energy transfers including the ring-to-ring and
conical energy transfers, and the energy fluxes of the perpendicular and
parallel components of the velocity field. We show that the rings with higher
polar angles transfer energy to ones with lower polar angles. For large
interaction parameters, the dominant energy transfer takes place near the
equator (polar angle $\theta \approx \frac{\pi}{2}$). The energy transfers are
local both in wavenumbers and angles. The energy flux of the perpendicular
component is predominantly from higher to lower wavenumbers (inverse cascade of
energy), while that of the parallel component is from lower to higher
wavenumbers (forward cascade of energy). Our results are consistent with
earlier results, which indicate quasi two-dimensionalization of quasi-static
magnetohydrodynamic (MHD) flows at high interaction parameters.
