Formation of Hot Closed Magnetic Structures / Loops in Solar Atmosphare with Account of Partially Ionized Gas Effects

In this study we consider the formation of hot closed magnetic structures / loops in Solar Atmosphere with account of partially ionized gas effects. In our model we assume the existence of large amount of neutrals, according to latest observations. We performed the numerical experiments for partially ionized situation to mimic the hot coronal loop formation phenomenon under the realistic observationally justified conditions. We constructed the solutions for realistic characteristic parameters and compared them to simple, fully ionized situation. The dependance of characteristic physical parameters on the boundary conditions including the time-dependent ones is shown. The results are promising, especially in view of the latest observational data on solar atmosphere.