We discuss here several effects of strong magnetic fields on the synth
esis of light elements during the big-bang. They include: changes in t
he reaction rates, variation in the expansion rate of the Universe, pa
rticle masses shift and the modification of the thermodynamical proper
ties of the QED plasma. Including these effects in the standard nucleo
synthesis code we are able to discriminate their relative importance.
Comparing our results with the observation we find that the allowed in
tensity of inhomogeneous fields at the end of the nucleosynthesis is 3
x10(10) Gauss.