  Recently it was shown that classical electromagnetism admits new asymptotic
conservation laws \cite{2007.03627}. In this paper we derive the analogue of
the first of these asymptotic conservation laws upon imposing Feynman boundary
condition on the radiative field. We also show that the Feynman solution at
$\mathcal{O}(e^3)$ contains purely imaginary modes falling off as $\lbrace
\frac{\log u}{u^nr}, n\geq 0\rbrace$ which are absent in the retarded solution.
The $\log u$ mode has also appeared in \cite{1903.09133,1912.10229} and
violates the Ashtekar-Struebel fall offs for the radiative field\cite{AS}. We
expect that new $\frac{(\log u)^m}{u^mr}$-modes would appear in the Feynman
solution at order $\mathcal{O}(e^{2m+1})$. Thus, all the other modes are
expected to preserve the Ashtekar-Struebel fall offs.
