We report a generalization of our earlier formalism [Pramana, 54, 663 (1998)] to obtain exact solutions of Einstein-Maxwell’s equations for static spheres filled with a charged fluid having anisotropic pressure and of null conductivity. Defining new variables: w=(4π/3)(ρ+ε)r², u=4πξr², v_r=4πp_rr², v_⊥=4πp_⊥r²[ρ, ξ(=−(1/2)F₁₄F¹⁴), p_r, p_⊥ being respectively the energy densities of matter and electrostatic fields, radial and transverse fluid pressures whereas ε denotes the eigenvalue of the conformal Weyl tensor and interpreted as the energy density of the free gravitational field], we have recast Einstein’s field equations into a form easy to integrate. Since the system is underdetermined we make the following assumptions to solve the field equations (i) u=v_r=(a²/2κ)rⁿ⁺², v_⊥=k₁v_r, w=k₂v_r; a², n(>0), k₁, k₂ being constants with κ=((k₁+2)/3+k₂) and (ii) w+u=(b²/2)rⁿ⁺², u=v_r, v_⊥−v_r=k, with b and k as constants. In both cases the field equations are integrated completely. The first solution is regular in the metric as well as physical variables for all values of n>0. Even though the second solution contains terms like k/r² since Q(0)=0 it is argued that the pressure anisotropy, caused by the electric flux near the centre, can be made to vanish reducing it to the generalized Cooperstock-de la Cruz solution given in [14]. The interior solutions are shown to match with the exterior Reissner-Nordstrom solution over a fixed boundary.