The Orion Kleinmann-Low nebula (Orion KL) is notoriously complex and exhibits a range of physical chemical components. We conducted high angular resolution (sub-arcsecond) observations $^13$CH$_{3}$OH $\nu=0$ ($\sim$0.3$^{\prime\prime}$ $\sim$0.7$^{\prime\prime}$) CH$_3$CN $\nu_8=1$ ($\sim$0.2$^{\prime\prime}$ $\sim$0.9$^{\prime\prime}$) line emission with the Atacama Large Millimeter/submillim...