The Griffiths Swarm-Integrated Mining Architecture (SIMA)

The Griffiths Swarm‑Integrated Mining Architecture (SIMA) Defines the industrial‑metabolic extraction layer of the Griffiths Canon It establishes the first fully autonomous, swarm‑integrated mining system designed for microgravity resource fields, enabling continuous extraction, in‑situ processing, and packetized material routing across asteroids, regolith bodies, and volatile‑rich environments. SIMA introduces a distributed industrial organism composed of micro‑extractors, macro‑burrowers, resonant fracture units, volatile capture drones, and localized processing nodes. These agents operate under DIGSP‑aligned behavioural rules, forming a self‑balancing, self‑healing swarm capable of adapting to substrate composition, thermal conditions, and kinetic hazards in real time. The architecture formalizes: swarm typologies and behavioural logic extraction methodologies across metallic, silicate, volatile, and rubble‑pile fields in‑situ processing pathways for sorting, pre‑refinement, volatile stabilization, and packetization micro‑logistics interfaces for NGLS handover operational envelopes for gravity, thermal, radiative, and kinetic constraints cross‑architecture integration with NGLS, GNMT‑Drive, the Dual‑Ring Habitat, and DIGSP SIMA serves as the canon’s industrial keystone: the upstream metabolic engine that generates the raw material streams required for propulsion, habitat construction, shielding, and manufacturing. This v1.0 foundational release establishes SIMA’s system definition, performance envelopes, safety constraints, and canon‑wide integration logic, preparing the architecture for future expansions including refinery‑class modules, heavy‑lift return systems, and autonomous mining colonies.