Dyson-Schwinger equations determine the Green functions G r (α, L) in quantum field theory. Their solutions are triangular series in a coupling constant α and an external scale parameter L for a chosen amplitude r, with the order in L bounded by the order in the coupling.Perturbation theory calculates the first few orders in α. On the other hand, Dyson-Schwinger equations determine next-to {j} -leading log expansions, G r (α,M sums for any finite j a finite number of functions M in u. Here, u is the one-loop approximation to G r , for example, for the (inverse) propagator in massless Yukawa theory, u = αL/2. The leading logs come then from the trivial representation M(u) = [ • ](u) at j = 0 with p [ • ] 0[101] Note that in general, u ∝ αL. Since we mainly consider the Green function for the Yukawa fermion propagator, the proportionality factor is 1/2. For the QED photon self-energy Green function that is also considered in this paper, one finds u = 4/3 αL.