Distributions of atmospheric quantities at the Hετ = 1 height. Panels show the kernel density estimation as a function of height, column mass, temperature, and electron density at the τ = 1 height for the Hε rest wavelength. The distributions are separated by the type of Hε profile, as indicated in the legend: absorption in HNEI, emission in HNEI, emission in SE, and the Ca II H background continuum at Hε rest wavelength in HNEI.