STACKED LIVE WORKSPACES
Every receiver gets its own spectrum, band plan, waterfall, signal meter, tuning state, hold controls, and focus mode.
SCAN WITH FIVE RADIOS AT ONCE.
Turn one to eight RTL-SDR receivers into a coordinated Windows radio array. Partition channel scans across every radio, hold on simultaneous signals, manage frequency libraries, capture and replay raw IQ, decode live traffic, connect remote receivers, and feed external radio tools.
SPECTER SDR treats every connected receiver as part of one instrument. Each radio keeps its own tuning, gain, antenna role, bearing, squelch, DSP calibration, waveform holds, and recording tracks while the workstation gives you one synchronized operational view.
Real controls, real local processing, and a workflow built for long monitoring sessions rather than quick single-radio checks.
Every receiver gets its own spectrum, band plan, waterfall, signal meter, tuning state, hold controls, and focus mode.
NFM, WFM, AM, DSB, LSB, USB, CW, and RAW modes with bandwidth, filter, shift, gain, squelch, and calibration controls.
Compare simultaneous events across antennas, infer direction from amplitude relationships, and flag movement across the array.
Define frequency ranges and dB-over-floor thresholds per receiver, preserve peaks, and clear individual or array-wide holds.
Hear every active receiver through one mixer with channel volume, mute, solo, live meters, and a master output.
Build Notice, Alert, and Critical classes by threshold and band, then capture synchronized waveform evidence when they fire.
Split 24-1766 MHz across the connected array and stitch each receiver slice into one faster combined spectrum and waterfall.
Render spectrum interpolation and waterfall palettes through WebGL2, with automatic high-performance canvas fallback.
Choose a frequency range or a saved channel group. SPECTER SDR partitions the work across the connected array, attributes every hit to the receiver that heard it, and leaves a dedicated ADS-B radio untouched.
Split contiguous ranges or saved channel groups across every available receiver.
Pause each radio independently while active transmissions remain above the configured floor.
Revisit priority channels, skip current activity, and persist nuisance-frequency lockouts.
Store time, frequency, strength, duration, detected CTCSS tone, and receiver identity.
Move frequency lists, raw signal recordings, remote radios, aircraft data, audio, and tuning commands through established radio formats and protocols.
Search and group named frequencies, tune on double-click, and import or export CSV lists.
Detect all 38 standard PL tones, filter NFM audio by tone, and stamp tones onto scanner hits.
Record gapless cu8 baseband, then replay cu8 or cf32 files at real-time pace with metadata restored.
Add roof, field, or network receivers as full array elements with forwarded tuning and gain controls.
Feed decoded aircraft over BaseStation TCP and stream a receiver's MP3 audio to an Icecast mount.
Let hamlib-compatible software read and retune a chosen SPECTER receiver through a standard TCP endpoint.
Decoder Lab validates Mode-S and ADS-B aircraft telemetry, AX.25 and APRS packets, POCSAG paging, and NOAA SAME weather alerts through five built-in profiles. Supported live engines add rtl_433 devices, AIS Marine, DSD-FME digital-voice events, and NOAA APT processing.
1090.000000 MHz · ALT 28,900 FT · 446 KT · HDG 071°
144.390000 MHz · POSITION / STATUS FRAME
162.550000 MHz · ORIGINATOR / EVENT / LOCATION
The same receiver array powers the Rosebud radial display and Research Labs without leaving the local workstation.


Assign names, physical slots, antenna types, and bearings, then move the array to a dedicated Rosebud window or second display. One receiver renders as a full 360-degree waterfall; larger arrays add comparative direction and confidence.
Record one workspace or Rosebud composite, lossless timestamped spectrum tracks, and per-receiver BWF audio without spawning one video encoder per dongle.
Drop event markers during the run. Alert classes automatically preserve frequency-labeled waveforms and synchronized array views.
Replay post-roll clips, navigate the timeline, export selected ranges, and open the exact saved Gallery event from the alert dialog.
Generate printable HTML and PDF alert reports with signal metadata, session context, and embedded spectrum and waterfall evidence.

Reserve one receiver for continuous ADS-B monitoring or let periodic mode borrow an assigned radio for a 10-second check every minute. Traffic extends the window to 15 seconds, then the receiver returns to its previous tuning automatically.
Research Labs stays out of the normal workflow until enabled. When active, it learns the local RF environment, distributes search bands across available radios, and checks qualified events against ordinary explanations.
Learns each receiver's normal spectrum and flags explainable novelty, chirps, Doppler-like drift, hopping behavior, periodic bursts, and wideband events.
Assigns aerospace, digital discovery, or wide survey ranges across idle receivers, alternates sweep direction, and restores saved tuning when stopped.
Compares findings with known protocol bands, live aircraft, visible satellites, array confirmation, bearing, and apparent movement before assigning a review status.
No cloud service is required for receiver control, decoding, pattern analysis, alerting, correlation, recording, reports, or the local evidence library. Optional map tiles and satellite catalog updates use OpenStreetMap and CelesTrak when those features are requested. SPECTER Imaging integration is optional and limited to local alert and trigger handoff.
No subscription and no required cloud service.