Maps of the radiative losses, temperature, and parallel magnetic field for different heights in the solar atmosphere. Top row: derived radiative losses for the entire FOV for the first time-step. The first panel from the left represents the total radiative losses integrated over the chromosphere. The other three panels show the radiative losses integrated over the lower, middle, and upper chromosphere, respectively. Middle row: maps of the temperature for four different heights in the solar atmosphere. The height increases from left to right. Bottom row: maps of the parallel magnetic field for four different heights in the solar atmosphere. The height is increasing from left to right. The first panels in the middle and bottom rows represent the T and B_|| in the photosphere, respectively. The green contours indicate the area where kW m⁻² in the corresponding atmosphere layer, where is the median value of Q in the corresponding layer. Const = 1.6 for the lower and middle chromosphere, and const = 0.7 for the upper layer.