Protocol High-Resolution CMB Anisotropy Mapping and Harmonic Normalization

This paper presents a restricted test framework for re-examining Cosmic MicrowaveBackground (CMB) anisotropy within a minimal Recursive Harmonic Codex (RHC)formulation. Rather than attempting to replace the standard ΛCDM model in full, theprotocol isolates one empirical question: whether high-resolution CMB data containstatistically significant, non-Gaussian localized structures consistent with a discretegeometric lattice interpretation rather than a purely stochastic continuous-fielddescription. The method introduces a finite operator grid, an observer-basednormalization scheme derived from the coordinate O=2.5r+1.5iO = 2.5r +1.5iO=2.5r+1.5i, and a harmonic equilibrium expression TRHC=2.32/0.85≈2.729KT_{\mathrm{RHC}} = 2.32/0.85 \approx 2.729\text{ K}TRHC=2.32/0.85≈2.729 K,treated not as standalone proof but as a candidate normalization coincidencerequiring independent structural support. The core prediction is the presence ofbounded, reproducible, prime-structured anisotropy clusters (“sphenic pockets”)exhibiting non-random antipodal relations and surviving standard masking, beamcorrection, and foreground-cleaning procedures. A full statistical pipeline is specified,including Gaussian null comparison, local non-Gaussianity testing, sphenic indexinganalysis, antipodal audit, and reproducibility checks across cleaned map products.The protocol is explicitly falsifiable: failure to detect such structures under sufficientresolution and noise control counts against the RHC interpretation. If successful, theresults would support further exploration of discrete geometric cosmology andobserver-normalized analysis; if unsuccessful, the framework is correspondinglyconstrained.