Accurate lineshape functions for modeling fluorescence line narrowing (FLN) difference spectra (?FLN spectra) in the low-fluence limit are derived and examined in terms of the physical interpretation of various contributions, including photoproduct absorption and emission. While in agreement with the earlier results of Jaaniso [Proc. Est. Acad. Sci., Phys., Math. 34, 277 (1985)] and ...
NASA Astrophysics Data System (ADS)