Abstract
- This specification details the structural layout, electromagnetic matrix parameters, and multi-phase fluidic propulsion models required to construct a non-mechanical Magnetohydrodynamic (MHD) Cymatic Thruster. Traditional atmospheric and space propulsion systems rely on mechanical compressors, physical fan blades, or high-friction rocket nozzles that succumb to rapid structural melting, bearing seizure, and material failure when exposed to extreme thermal loads (745 K) and crushing ambient pressures (9.5 MPa).
SPEC-285-CORE resolves these mechanical constraints by implementing an active, electromagnetic working-fluid pump grid natively integrated within the TECTONEX chassis panels. By ionizing incoming high-density supercritical carbon dioxide (scCO2) or interstellar plasma streams via high-frequency Gallium Nitride (GaN) power stages, the medium is accelerated through interior conduits lined with additively manufactured permanent magnetic arrays. Governed strictly by the Lorentz vector cross-product and anchored to the master Covariant Dynamic Sieve (CDS) network function, this design converts environmental resistance directly into stabilizing structural thrust, providing an open prior-art blueprint for zero-moving-part, high-velocity planetary exploration initiatives.
Creative Commons License
This work is licensed under a Creative Commons Attribution 4.0 License.
Recommended Citation
Eckes, Christopher L., "TECHNICAL DISCLOSURE SPECIFICATION: SPEC-285-CORE TITLE: MAGNETOHYDRODYNAMIC CYMATIC THRUSTER DESIGN AND PLASMA FIELD COUPLING: TRANSVERSE KINETIC ENERGY HARVESTING CAVITIES UTILIZING PROPULSION METRICS FOR ADVANCED SPACEFRAME EXPLORATION", Technical Disclosure Commons, (October 28, 2026)
https://www.tdcommons.org/dpubs_series/12504