We have made simultaneous measurements of the longitudinal and transverse NMR frequencies of He-A in fields of the order of 30 G in a parallel plate geometry, defined by Mylar films 100pm apart, so that 1 is well oriented perpendicular to the static magnetic field. Comparison of our measurements with the quadratic axial-state frequency relation indicates that the A phase is axial in the pressure range 22.6 to 29.3bars. PACS numbers: 67.57.Lm, 76.60.Jx It has recently been suggested [1,2] that the conventional identification of the Cooper pair state in the A phase of superfluid 3He with the Anderson-Brinkman-Morel [3] (or axial) state might be incorrect. Experimental information on the generalized Ginzburg-Landaufourth-order free energy coefficients pl, pz, ps, p4, and p5 suggests that the axiplanar state [4] might be more stable than the axial state over at least part of the A-phase region of the phase diagram. In addition, our own measurements of the A-phase superfluid density anisotropy at 29.3 bars [5] give a value for (p,~-ps~~) /p,~o f 0.42 +0.03 as T~T~, this represents a possibly significant departure from the value of 0.5 predicted for the axial state in the direction expected for an axiplanar order parameter. At the melting pressure strong coupling corrections [6] make the predicted anisotropy for the axial state slightly larger, 0.515.Since the identification of the A phase with the axial state is the basis for much theoretical work and also for the interpretation of a substantial number of experiments, it is important that its validity should be thoroughly checked and that was the purpose of the work described in this Letter. The relationship between the longitudinal and transverse NMR frequencies, O~~a nd Ag, of the A phase provides a precise method for doing this. For t;he axial state in an applied magnetic Beld there is a simple quadratic relation between these frequencies ll 2 2 w here AL, is the Larmor frequency of the He nucleus. For the axiplanar state O~e xceeds 0& -0& by an amount which measures the cleparture of the order parameter from the axial form. Previously, Eq.(1) has been checked carefully only at the melting pressure 34.3 bars, [7] where the identification of the A phase with the axial state seems secure. The axiplanar order parameter is specified by angles 8 and P and it can conveniently be written in terms of the spin-space unit vector triad (d, e, f) and orbit-space unit vector triad (1, m, fl) [8] as proportional to We see that spin-up and spin-down states have diferent orbital anisotropy axes at angles +P to 1; the axial phase corresponds to the limit P~0 , 8~z/4. For P g 0 and 8 P z/4 expression (2) indicates a state with a coherent sum of orbital angular momentum up and down for each spin state.The axiplanar state is more stable than the axial state if p45 = p4 + ps ) 0, in which case the angles p and 8 are given in terms of the P's by [4] tan 2P13P45 P345(2PI + Ps)' cos 8= P3(2Pl + P345) 2[Ps(2P1 + P345) + P45(2P1 + P3)](3) We note that in the limit T~Tc the order parameter(2...