Protocol & Results Introduction This document formally describes the Near-Surface Solar Magnetic/EMF–Ӕ Cross-Check protocol, its execution using canonical default parameters, and the results obtained. The purpose of this work is to test whether the Ӕ model can predict the photoning depth (r*) of the solar photosphere with a fixed set of constants derived independently from…

Our SolarMagnetic Field Project The Lowdown Introduction This document outlines our Angle of Encounter (Ӕ) model test for predicting the photoning depth (r*) of the Sun’s photosphere, crafted for student physicists with the aim of clarity, rigor and replicability. The Plan The project follows a two-step process:1. Calibration – Using independent limb-darkening data to derive…

Our SolarMagnetic Field Project Introduction This project tests whether our Angle of Encounter (Ӕ) model can predict the “photoning depth” (r*) of the Sun’s photosphere, the depth below the visible surface where photons emerge. The question is whether we can use measured magnetic field data to locate this depth precisely, without tuning the model after…

Matching NASA’s Gravity Probe B Without Curving Space-Time Background In 2004–2011, NASA’s Gravity Probe B (GP-B) mission measured the geodetic effect, the precession of a gyroscope in orbit around Earth, with unprecedented precision: 39.2 milliarcseconds per year (mas/yr), within ±0.5 mas/yr of General Relativity’s prediction. GP-B was a technological masterpiece, costing over $750 million and…