Abstract
The observations and identifications of the chromospheric evaporation of solar flares during the 21st solar peak years are considered a great discovery in the history of solar physics. In order to explain the process of chromospheric evaporation,many hydrodynamical models of solar flares have been proposed. These models can explain chromospheric evaporation and predict that there should exist some chromospheric material moving downward, responding to the flare energy release. This downward moving chromospheric material, usually named chromospheric condensation, has a structure
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