The Woomera Observation:In the early 1960s, radar observations at the Woomera Rocket Range in South Australia, operated by the Weapons Research Establishment (WRE), detected a significant signal that contributed to the development of TSM2.0. While tracking ionospheric anomalies—transient signals termed “Angles” caused by plasma-based ionization domains—the radar systems identified a uniform 3.5 K signal present in all directions. Initially dismissed as noise, systematic elimination of terrestrial sources confirmed its cosmic origin, mirroring the characteristics of the CMB later identified by Penzias and Wilson in 1965.
This observation, shared through international collaborations, highlighted the potential for wave-based phenomena to uniform cosmology. The uniform signal challenged the Standard Model’s reliance on a very small, very hot, very dense singularity, prompting the exploration of a wave-driven framework starting from a very large, very cold, very diffuse massive field, the Net-Zero-Energy-Field (NZEF) TSM2.0 leverages such observations to propose a cosmos where scalar field fluctuations and gravitational warping, through wave dynamics, give rise to the structured universe, providing a more integrated explanation for phenomena like the CMB (Chapter 7).
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