Parameters of sensitivity of Fraunhofer lines to changes in the temperature, gas pressure, and microturbulent velocity in the solar photosphere
Parameters are proposed for measuring the sensitivity of Fraunhofer lines to the physical conditions in the solar atmosphere. The parameters are calculated based on depression response functions in the LTE approximation. The sensitivity of lines to the temperature, gas pressure, and microturbulent velocity depending on the line and atomic parameters is investigated. The greatest relative temperature sensitivity is shown by weak lines, while the greatest absolute sensitivity is displayed by moderate lines of abundant heavy atoms with low ionization and excitation potentials. The excitation potential and line strength are the crucial factors for the temperature sensitivity. The highest pressure sensitivity is observed for moderate lines of light atoms with very high excitation potentials (exceeding 6 eV), and strong photospheric lines (8 pm < W < 14 pm) of heavy atoms are the most responsive to the microturbulent velocity. The sensitivity parameters can be also used to advantage for physical diagnostics of the photosphere when the temperature, pressure, and microturbulent velocity fluctuations are no more than 8%, 50%, and 100%, respectively.