The Founding Axis: Profile Shape, Transfer, and Direction for the Large-Angle Cosmic Microwave Background

Paper 1 of 3 in the CMB anomalies series. The torsion-regulated bounce framework carries an inherited axis at every founding, and a companion analysis proved the morphology theorem: an axisymmetric founding profile gives the quadrupole and octopole a shared axis identically. This paper attacks the three missing pieces that stood between that theorem and a mechanism for the observed sky. Profile shape: three routes through the framework's owned machinery each fail at the marking law, which remains the named missing object; the amplitudes are not derived. What is derived instead is the profile's dispersion structure (the dispersion vanishes about the founding axis and is maximal on its equatorial circle) and the sectoral bound: for the dispersion axis to sit on the symmetry axis, the octopole must carry a sectoral component of at least 0.80 of the axial power and the quadrupole at least 3.00 (9.00 for planarity 0.90), where the framework today owns exactly zero; the two owned candidate structures for that component are examined and both are obstructed by axisymmetry. Transfer: derived for structure (every verdict survives any admissible transfer), unowned for amplitudes. Direction: the orientation law determines the axis as a vector, three directional tests are pre-registered, and the current galaxy-spin literature is printed in full as adverse-to-neutral. The scar-handedness toll is stated in the only terms available before the marking law: sign, statistics, thresholds, and controls (Monte Carlo nulls SIMULATED, NOT MEASURED). Deposited manuscript: register-corrected version (wording only; every number unchanged).