Emission spectroscopy as one of the standard methods to measure atomic
transition probabilities is discussed with its advantages, its restri
ctions and its pitfalls. The measurement of branching fractions combin
ed with lifetime data obtained with modern laser techniques is discuss
ed as the prevailing measuring procedure which guarantees large sets o
f reliable f-values. The trend to shorter wavelengths in astrophysics
and in fusion research will also in the future keep emission spectrosc
opy attractive.