CRITICAL FART SIGNAL DETECTED
LIVE DATA FEEDS: GWOSC ○ NASA DONKI ○ NEUTRINO-SAT ◎ SIMULATED DRAG CURSOR ON RADAR TO PROBE · CLICK TO INJECT SIGNAL
RA: --- DEC: --- DIST: --- SIGNAL: --- SPECIES: ---
SPECTROGRAM // REAL-TIME FOURIER TRANSFORM
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DOMINANT FREQ
Hz
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AMPLITUDE
dB normalised
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BANDWIDTH
Hz (FWHM)
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SNR RATIO
dB
SIGNAL-TO-TONE MAPPING
PARAMETERMAPPED TORANGE
Signal strengthOscillator frequency80–2400 Hz
Methane %Filter cutoff200–8000 Hz
Distance (Mpc)Reverb decay0.1–4.0 s
Sulfur %Distortion gain1.0–20.0
Quantum gas %LFO rate0.1–12 Hz
Species classWaveform typesine/sq/tri/saw
Threat levelMaster gain0.1–1.0
SYNTHESISER // MANUAL SIGNAL GENERATION
SPECIES SIGNAL TONES // CLICK TO AUDITION
PIANO ROLL // RECENT DETECTIONS
REALTIME CONTROLS
60
40
30
REAL-WORLD DATA FEEDSLOADING...
GWOSC (Gravitational Wave Open Science Center)
Fetching latest gravitational wave events...
NEUTRINO-SAT PRIME // SIMULATEDONLINE
NEUTRINO-SAT-1 // L4 LAGRANGE POINT
NEUTRINO FLUX DENSITY
0.00
× 10⁻¹² cm⁻² s⁻¹ sr⁻¹
SIM
METHANE COLUMN DENSITY
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Mean galactic methane anomaly index via NIRD spectroscopy
UPDATE INTERVAL: 4.2s // RESOLUTION: 0.03 arc-sec
SIM
SONIC PRESSURE WAVE EVENTS
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Sub-Hz pressure anomalies propagating through interstellar medium
LAST 24H // THRESHOLD: 10⁻¹⁸ Pa
SIM
QUANTUM ENTANGLEMENT FUMES
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Entangled gas molecule pair detection (non-classical correlation ≥ 0.82)
BELL INEQUALITY VIOLATION INDEX
EVENT TIMELINELOADING NASA...
NASA DONKI // SPACE WEATHER
Fetching NASA space weather data...
GFSD-9000 v2
GALACTIC FART SIGNAL DETECTOR // TECHNICAL DOCUMENTATION // HEART OF GOLD INTELLIGENCE DIVISION

01 — SYSTEM OVERVIEW

The GFSD-9000 is a geospatial intelligence platform for the real-time detection, classification, and sonification of bio-sonic anomaly signals originating from galactic distances of up to 1,000,000 parsecs (approximately 3.26 million light-years). The system integrates real-world space science data feeds with a forward-looking neutrino-radar detection architecture designed for the advanced detection of minute element fluctuation anomalies propagated through interstellar and intergalactic media.

OPERATOR NOTE (BEEBELBROX PROTOCOL): This system is calibrated for the specific acoustic and chemical fingerprint of bio-sonic expulsion events (colloquially: farts) across all known intelligent species within the observable Local Group. Classification accuracy degrades beyond 800,000 parsecs due to cosmic microwave background interference.

The interface provides four operational modes: the primary Scanner view with live radar overlay; the Sonification Engine for acoustic intelligence analysis; the Satellite Data dashboard for real and simulated feed integration; and this technical documentation.

02 — REAL-WORLD DATA SOURCES

While no publicly available API currently provides galactic fart signal data specifically (a gap we consider unconscionable), the GFSD-9000 integrates with two real open-data sources whose anomaly signatures are repurposed as fart-proxy signals. Both APIs are freely accessible without authentication.

GRAVITATIONAL WAVE OPEN SCIENCE CENTER (GWOSC)

The GWOSC provides public access to strain data from the LIGO, Virgo, and KAGRA gravitational wave observatory network. Detected merger events (black holes, neutron stars) are re-classified by our AI as high-energy quantum-phase fart events — because at sub-parsec scales, the distinction is largely philosophical.

GET https://gwosc.org/eventapi/json/allevents/ Full gravitational wave event catalog
GET https://gwosc.org/eventapi/json/query/?release=GWTC-3 Third observing run catalog
DATA MAPPING: GWOSC events are ingested and their strain values (10⁻²¹ m/m) are mapped to our signal strength scale (dBm). Event luminosity distance (Mpc) maps directly to radar distance. Source classification (BBH, BNS, NSBH) maps to our species taxonomy. Chirp mass maps to methane concentration index.

NASA DONKI (SPACE WEATHER DATABASE)

NASA's DONKI API provides real-time solar and space weather event data including coronal mass ejections (CMEs), solar flares, geomagnetic storms, and radiation belt enhancements. These solar plasma expulsions are, obviously, the sun's farts — and are classified as a Class-G VOGON-SOLAR signal type in our taxonomy.

GET https://api.nasa.gov/DONKI/CME?startDate=YYYY-MM-DD&api_key=DEMO_KEY Coronal mass ejection events (solar farts)
GET https://api.nasa.gov/DONKI/FLR?api_key=DEMO_KEY Solar flare events (sonic component)
GET https://api.nasa.gov/planetary/apod?api_key=DEMO_KEY Astronomy picture — used for background ambience seeding
DATA SOURCESTATUSAUTH REQUIREDRATE LIMITFART PROXY TYPE
GWOSC Events API✓ LIVENoneNone statedQuantum-phase fart
NASA DONKI CME✓ LIVEOptional (DEMO_KEY)1000/hrVogon-solar fart
NASA DONKI FLR✓ LIVEOptional (DEMO_KEY)1000/hrSonic burst component
NEUTRINO-SAT PRIME◎ SIMULATEDFuture: HMAC-SHA256N/AAll types

03 — NEUTRINO-SAT ARCHITECTURE // FUTURE PRODUCTION SYSTEM

The production NEUTRINO-SAT constellation is a proposed deep-space sensor network designed specifically for the detection of bio-sonic anomaly signatures at galactic scale. The following specifications represent the envisioned system for deployment circa 2031–2035.

NEUTRINO-SAT PRIME // ORBITAL SPECIFICATIONS

Orbital PositionSun-Earth L4 Lagrange Point (60° ahead of Earth)
Constellation Size3 primary nodes + 12 relay micro-sats
Baseline Separation2.5 × 10⁹ km (interferometric baseline)
Mission Lifetime15 years (extendable)
Launch VehicleHeart of Gold Improbability Drive Mk.IV

DETECTION TECHNOLOGY // NEUTRINO-EMISSION RADAR (NER)

Primary SensorMuon neutrino tomography array (10⁶ channels)
Detection MechanismCoherent elastic neutrino-nucleus scattering (CEνNS)
Neutrino Energy Range5 MeV – 100 GeV (broadband)
Angular Resolution0.03 arc-seconds at 1 Mpc
Max Detection Range1.2 × 10⁶ parsecs (Local Group limit)
Sensitivity10⁻¹² cm⁻² s⁻¹ sr⁻¹ (flux density)
HOW NEUTRINO-RADAR DETECTS FARTS THROUGH MATTER: Unlike electromagnetic radiation, neutrinos pass through virtually all matter — planets, star cores, entire galaxies — with negligible absorption. The NEUTRINO-SAT system actively pulses a directional neutrino beam (via stimulated weak-force emission from an enriched muon-catalysis chamber) and measures the backscatter coherence pattern. Bio-sonic events produce a unique chemical trail of CH₄/H₂S/volatile organics that modulates the neutrino cross-section at 10⁻⁴³ cm² resolution. The system can thus detect a Vogon flatulence event from behind a neutron star at 800,000 parsecs.

SIGNAL PROPAGATION MODEL

Fart signals propagate through the interstellar medium via three distinct channels: (1) acoustic pressure waves through dense molecular clouds (range: ~50 light-years), (2) chemical tracer diffusion detectable by molecular spectroscopy (range: ~10,000 light-years), and (3) neutrino-modulated quantum coherence signatures detectable by NEUTRINO-SAT (range: ~1,000,000 parsecs). The GFSD-9000 integrates all three channels.

CHANNELPROPAGATION MEDIUMMAX RANGELATENCYRESOLUTION
AcousticISM molecular clouds50 ly50 yearsHigh (chemical detail)
SpectroscopicH-alpha + CH₄ bands10,000 ly10,000 yearsMedium (species ID)
Neutrino coherenceAll media (penetrating)1,000,000 pc3.26M yearsLow (event confirmed)

04 — DETECTION METHODOLOGY

The GFSD-9000 radar uses a rotating synthetic aperture neutrino beam sweep. The sweep arm rotates at a configurable rate (0.125–1.5 Hz) and paints the galactic sphere with a coherent neutrino pulse. Returns are processed by a matched-filter bank tuned to 42 known bio-sonic spectral templates (one for each answer to the ultimate question).

Signal classification uses a multi-stage pipeline: (1) threshold detection at -90 dBm, (2) spectral fingerprinting against species library, (3) chemical composition decomposition (methane/sulfur/bio-toxin/quantum-gas/sonic), and (4) threat-level assignment based on combined intensity and proximity weighting.

THREAT CLASSIFICATION MATRIX

LEVELdBm RANGEDISTANCECOMPOSITIONRESPONSE
NOMINAL< -70 dBm> 500 kpcStandardLog only
ELEVATED-70 to -50 dBm50–500 kpcElevated CH₄Alert + audio
CRITICAL-50 to -30 dBm1–50 kpcHigh H₂S + sonicEmergency tone
MAXIMUM> -30 dBm< 1 kpcAll agentsDon't panic

05 — DATA SONIFICATION ENGINE

The sonification system uses the Web Audio API to translate multi-dimensional signal data into a real-time auditory experience. Each detection event generates a synthesised tone whose acoustic properties are fully determined by the signal's measured parameters.

FREQUENCY MAPPING

Signal strength (dBm) maps logarithmically to oscillator frequency: freq = 80 * Math.pow(2400/80, (signal+90)/60) Hz, spanning 80 Hz (weakest detectable) to 2400 Hz (maximum threat). This places Vogon bureaucratic fart signals in the uncomfortable 800–1200 Hz band, as is scientifically appropriate.

CHAIN ARCHITECTURE

The synthesis chain consists of: Oscillator → Gain (velocity) → BiquadFilter (methane-modulated) → WaveShaper (sulfur distortion) → ConvolverNode (space reverb) → DynamicsCompressor → Analyser → MasterGain → AudioContext.destination. A secondary LFO oscillator modulates filter cutoff at a rate set by quantum-gas concentration.

CLICK AUDIO ON/OFF in the Scanner tab or use the SONIFICATION tab to audition individual species tones. All synthesis happens client-side — no audio data is transmitted. The system requires user interaction to initialise the AudioContext per Web Audio API browser policy.

06 — SIGNAL CLASSIFICATION TAXONOMY

CLASSDESIGNATIONINDICATORTYPICAL RANGENOTES
GAS-CLOUD-7Distributed methane nebulaSlow rise, long tail100–500 kpcUsually harmless
METHANE-BURSTAcute CH₄ detonationSharp spike, fast decay10–100 kpcAvoid open flames
SULFURIC-WAVEH₂S broadband emissionWide spectrum, low freq50–200 kpcOlfactory hazard
QUANTUM-TOOTNon-classical entangled gasNon-local correlationAnySpooky action
BIO-SONICAcoustic pressure eventNarrow freq, high Q<50 kpcDirect weapon use
SILENT-BUT-DEADLYLow-emission, high-toxinVery weak signal, max bio1–20 kpcCRITICAL THREAT
HYPERSPACE-FUMEDimensional bleed eventDiscontinuous signatureAnyImprobability drive

07 — FUTURE PRODUCTION API REFERENCE

The following endpoints are planned for the NEUTRINO-SAT Ground Control API (production deployment 2031). All endpoints return JSON. Authentication uses HMAC-SHA256 with rotating 42-second keys.

GET/api/v1/scan/liveCurrent sweep data, all contacts
WSwss://neutrino-sat.heartofgold.int/streamReal-time signal stream (WebSocket)
GET/api/v1/events?since=ISO8601&range=parsecsHistorical event log with filtering
GET/api/v1/composition/{eventId}Full chemical decomposition of a signal
GET/api/v1/neutrino/flux?ra=DEG&dec=DEG&r=PCPoint-source neutrino flux query
GET/api/v1/species/identify?fingerprint=BASE64Species classification from spectral fingerprint

08 — KNOWN SPECIES ACOUSTIC SIGNATURES

SPECIESWAVEFORMFREQ (Hz)CH₄%H₂S%NOTES
VOGONSquare120–1804538Weaponised. Poetry precedes event.
ZAPHOD-CLASSSawtooth280–4203022Two-headed dual-emission pattern
MARVIN-PATTERNSine (depressed)421815Low energy. Brain the size of a planet.
SLARTIBARTFASTTriangle600–800528Fjord-shaped spectral peaks
TRILLIANSine (clean)440–660125Highly refined. Almost musical.
ARTHUR-DENTNoisy sine200–3502818Confused. Mostly harmless.
BUGBLATTER BEASTSawtooth (distorted)30–807865Cannot see you if you cover your eyes
⚠ WARNING: If you detect a VOGON signal above -50 dBm, do NOT attempt diplomatic communication. Their poetry is classified as a separate bio-hazard event and will trigger an additional SONIC-BURST classification. Flee at improbable speeds.
GFSD-9000> AWAITING SIGNAL... CONTACTS: 0 DATA: SIM AUDIO: OFF