AI Studio Architecture
Two-system architecture separating production AI services from design and development workloads. All machines connected via 10Gb backbone with SSH key-based orchestration.
- i9-10900K · 32 GB DDR4 · RTX 2080 Super 8GB
- Ubuntu 24.04 LTS · Headless
- Open WebUI · AnythingLLM · n8n (Docker)
- Faster-Whisper STT (CUDA int8)
- Storage: 2.3 TB (NVMe + LVM)
- Ollama: 6 models including custom NIK persona
- i9-10980HK · 32 GB DDR4 · RTX 3080 16GB
- Linux Mint 22.3 · Kernel 6.17
- TeslaQuake data collectors deployed
- NOAA SWPC + INTERMAGNET processing
- Storage: 2.8 TB across 3× NVMe
- Battery UPS — surge-protected, sleep disabled
- i9-13900KS · 64 GB DDR5 · RTX 4090 24GB
- Windows 11 Pro · CUDA 13.2 · 10Gb SFP+
- IRIS: custom Gemma4:31b vision model
- Ollama: 7 models (181 GB total)
- Llama3.2-vision:90b, Llama3.3:70b
- Swappable between System 1 and System 2
- i9-14900KF · 64 GB DDR5 · RTX 4090 24GB
- Windows 11 Pro · 3-monitor setup
- Claude Code + Claude Desktop
- TeslaCoder v3 dashboard host
- SSH keys to all machines (silent auth)
- i9-12900KF · 32 GB DDR5 · RTX 3080 Ti 12GB · Linux Mint 22.3
- FreeCAD (2D permits + 3D design) · Blender 4.0 (photorealistic renders) · Direct 10Gb DAC link to Forge for heavy render offload
Data Inventory — 13 Monitoring Categories
563 GB of geophysical data collected across 80,000+ files, distributed between NIK and ECHO machines. Spanning solar, geomagnetic, Schumann resonance, telluric, ionospheric, seismic, atmospheric, bioacoustic, and more — with some datasets reaching back to 1934.
| Category | Research Factor | Total Size | Files | Coverage | Gap Status |
|---|---|---|---|---|---|
| Solar / Geomagnetic | W | 58.1 GB | 20,085 | 1963–2026 | No gaps in analysis window |
| Schumann Resonance | R | 35.3 GB | 36,091 | 2000–2026 | 20 gap years (1980–1999) |
| Telluric | T | 28.2 GB | 5,941 | 2005–2026 | 31 gap years |
| Ionospheric | I | 215.5 GB | 22,916 | 1950–2026 | No gaps in analysis window |
| Celestial | Z | 197.5 MB | 461 | 1900–2026 | 40 gap years |
| Seismic | S | 1.2 GB | 3,547 | 1990–2026 | No gaps in analysis window |
| Atmospheric | A | 140.8 GB | 5,178 | 1934–2026 | No gaps in analysis window |
| Bioacoustic | B | 75.8 GB | 10,289 | 2015–2025 | 37 gap years |
| Animal Behavior | AN | 7.6 GB | 1,716 | In collection | Emerging category |
| Ocean / Tidal | O | 400.5 MB | 1,175 | 1909–2025 | 35 gap years |
| Volcanic | V | 6.0 MB | 42 | 2026 | 46 gap years |
| Gravity | G | 118.1 MB | 21 | In collection | Emerging category |
| Events / GDACS | E | 1.1 GB | 457 | 2010–2026 | 30 gap years |
| Total | 563 GB | 107,919 | |||
Triple-Algorithm Anomaly Detection
Three complementary statistical algorithms running in parallel, each detecting different anomaly signatures. Combined output feeds a proprietary accumulation model protected under pending patent.
Welford
Online streaming algorithm computing mean and variance per metric, weekday, and month. Detects statistical spikes with z-score thresholds at 1.5 (low), 2.0 (medium), 3.0 (high), and 4.0 (critical). Requires minimum 10 samples before activation.
CUSUM
Two-sided cumulative sum for regime shift detection. Identifies sustained directional drift in metrics that may not trigger spike-based detectors. Complements Welford by detecting gradual rather than sudden changes.
EWMA
Exponentially weighted moving average with α=0.2 balancing reactivity and stability. Flags when smoothed trends breach control limits or sustained directional movement is detected. Provides trend context for the other two algorithms.
Database Architecture
108 PostgreSQL tables in Supabase managing real-time data ingestion, historical archives, anomaly detection state, and correlation analysis — migrating to fully local infrastructure.
- Active Tables: 108 in public schema
- Largest Tables: SuperMAG stations (943K rows), IERS polar motion (23K rows), Schumann readings (359K rows)
- Real-Time Feeds: NOAA Kp/Dst, GOES X-ray, solar wind plasma/mag, SWPC alerts (169K rows)
- Historical Archives: 358K historical earthquakes (25 years M4.0+), 76K daily sunspot numbers (1818–present)
- Anomaly State: 6,804 detected anomalies with z-scores, 16 CUSUM state records, 16 EWMA state records
- Migration: Transitioning from Supabase cloud to local PostgreSQL on NIK/ECHO
Source Provenance
All data sourced from established governmental, academic, and research institutions.
- USGS — Earthquake Hazards Program
- NOAA SWPC — Space Weather Prediction Center
- NASA OMNI — Merged solar wind data
- NASA CDDIS — IONEX ionospheric data
- NASA SDO — Solar Dynamics Observatory
- NASA DONKI — Space weather events
- GFZ Potsdam — Official Kp Index (1932–present)
- Kyoto WDC — Dst Index (1957–present)
- SILSO/ROB — Sunspot Number (1700–present)
- INTERMAGNET — Global magnetometer network
- SuperMAG — 943K+ station records
- HeartMath GCI — Schumann resonance monitoring
- Tomsk SOS-70 — Schumann observatory
- Cumiana VLF — VLF monitoring station
- IERS — Earth orientation parameters
- GDACS — Global disaster alerts
Research Objectives
The infrastructure is built. The data is flowing. These are the next steps that require institutional support, independent oversight, and peer collaboration.
Independent Peer Review
Submit correlation methodology and observation data to independent seismological and space weather researchers for formal peer review and publication in a refereed journal.
PriorityBlind Validation Study
Design and execute a prospective blind validation study with pre-registered methodology, time-stamped observations, and independent oversight to establish statistical significance.
PriorityExpanded Sensor Network
Deploy additional Schumann resonance and telluric monitoring stations to fill data gaps — particularly the 20-year Schumann gap (1980–1999) and 31-year telluric gap.
InfrastructureHistorical Backtesting
Complete formal backtesting across the 1980–2026 analysis window using the four gap-free categories (Solar, Ionospheric, Seismic, Atmospheric) against the full USGS M4.0+ historical record of 358,000+ events.
ValidationExplore the Research
Review our documented correlation events or discuss partnership opportunities.
Observation Log Research Partnerships