On the Aller's admixture radiation effect during the compression process in the solar corona and generation of coronal formations

The cooling due to Aller's admixture radiation in the energy balance equation describing the coronal gas condensation is taken into account. It is shown that the compression mechanism does not apply for the explanation of the quiescent prominences formation but is quite suitable for definite kinds of active prominences and flares of coronal origin.Two possible variants of magnetic field before and in the process of compression within the coronal element and beyond it are considered.