To first order in the deviation from scale invariance the inflationary
potential and its rst two derivatives can be expressed in terms of th
e spectral indices of the scalar and tensor perturbations, n and n(T),
and their contributions to the variance of the quadrupole CBR tempera
ture anisotropy, S and T. In addition, there is a ''consistency relati
on'' between these quantities: n(T) = -1/7 (T/S). We discuss the overa
ll strategy of perturbative reconstruction and derive the second-order
expressions for the inflationary potential and its first two derivati
ves and the first-order expression for its third derivative, all in te
rms of n, n(T), S, T, and dn/d ln k. We also obtain the second-order c
onsistency relation, n(T) = -1/7(T/S)[1 + 0.11(T/S) + 0.15(n - 1)]. As
an example we consider the exponential potential, the only known case
where exact analytic solutions for the perturbation spectra exist. We
reconstruct the potential via Taylor expansion (with coefficients cal
culated at both first and second order), and introduce the Pade approx
imant as a greatly improved alternative.