Real-time audio analysis and metering, wherever you work.
Prism is a free, open-source audio analyzer and meter rack for Windows, macOS, and Linux.
Monitor system audio or an input with a configurable set of real-time scopes and meters, arrange them however you like, and save the setup as a profile. The same analyzers are also available as VST3/AU/CLAP plugins, and Prism includes a native terminal interface for lightweight monitoring.
The desktop app's Channel Routing matrix works with system audio and device inputs on macOS, Windows, and Linux. Select any source channel independently for Prism's Left and Right channels, including the same channel for both. Activity fills show the incoming signal on every available channel, before routing and input trim; routes are saved per source.
Prism includes eight real-time scopes and meters:
- Spectrum Analyzer — FFT spectrum with calibrated dBFS levels, configurable FFT size, spectral tilt, Log/Mel/Linear scales, heatmap and fill modes, and peak/pitch readouts
- Oscilloscope — Time-domain waveform with fundamental-frequency pitch locking and sub-sample triggering for a stable display
- Vectorscope — Full-band stereo phase analysis with XY, Polar, and M/S Linear views, calibrated references, adjustable zoom, and optional multiband RGB
- Waterfall — Layered spectrum history with 1–30 seconds of audio, adaptive ridge density, theme or heat colors, and frequency/time guides in the desktop app, TUI, and DAW plugin
- Spectrogram — Scrolling frequency-over-time display with Log/Mel/Linear scales, stereo-energy analysis, and frequency reassignment in Sharp and Sharper modes
- VU Meter — 300 ms metering with adjustable 0 VU reference, stereo correlation, and needle or bar displays
- Loudness Meter — ITU-R BS.1770 momentary, short-term, and integrated LUFS metering with BS.1770 true-peak activity
- Waveform — Scrolling mono or stereo waveform with transient-preserving min/max sampling and optional multiband energy visualization
Every scope can be configured independently. Resize and rearrange them into a rack, rotate supported scopes, pop them into separate windows, or pin them on top of other applications.
On Windows, enable Reserve screen space in the rack's Top/Bottom reposition menu or its tray equivalent to dock the main rack across one monitor. Maximized applications use the remaining workspace. Resize the edge facing the workspace, drag the grab handle to return to a floating rack, or disable the option to restore its previous position and size. Settings open in a separate panel beside the dock. Docking is remembered on this computer independently of profiles; minimizing or hiding Prism releases the reserved space.
Spectrum, Spectrogram, Oscilloscope, and Waveform also include interactive measurement overlays for inspecting frequency, level, pitch, amplitude, or time directly from the display. Optional Linked Analysis mirrors compatible frequency, history-time, and amplitude guides across docked and detached scopes.
Stats for nerds
Most of Prism's analysis runs in native C++, with the same DSP implementations reused across the desktop app, DAW plugins, and terminal interface where applicable.
- Hann-windowed FFT with selectable sizes from 1024 to 16384 samples
- Coherent-gain correction for calibrated dBFS magnitude rather than arbitrary FFT amplitude
- Native calibration tests measure bin-centered tones within ±0.05 dB and off-bin interpolated peaks within 0.3 dB across all exposed FFT sizes
- Maintains Mid, Side, Left, Right, and channel-max spectra internally
- Logarithmic, Slaney Mel, and Linear frequency scales
- Extended 10 Hz–24 kHz and Audible 20 Hz–20 kHz ranges, automatically clamped to Nyquist
- Independent spectral and heatmap tilt around a 1 kHz reference
- Peak analysis can report dBFS, frequency, musical note, octave, and cents offset
- Interactive measurement overlay exposes frequency, level, and pitch directly from the graph
- One whole-track reference: drop a mono/stereo WAV, AIFF, FLAC, or MP3 onto the spectrum, or use Spectrum settings → Reference → Load track
- Dashed Overlay and a centered ±24 dB Difference view, with ±24 dB reference trim and one-shot Match level using the latest three seconds of live Mid audio
- Cancellable background analysis with an evolving preview; analyzed curves are saved with profiles and Spectrum plugin state, so recall does not need the original file
Spectrum settings have General and Reference tabs. Matching requires at least one second of current, non-silent audio. During import, the spectrum temporarily shows Overlay; the previous reference remains available if loading fails or is canceled. Reference analysis uses a shared 48 kHz path with all five FFT sizes cached, while respecting the original file's bandwidth. This affects analysis only.
- Independent native FFT analyzer with the same calibrated channel-max stereo spectrum as Spectrum
- Stores 60 spectrum slices per second on the audio clock, independent of terminal or desktop refresh rate
- Bounded 1–30 second history; defaults to 5 seconds
- Sparse, Balanced, and Dense ridge settings adapt to panel size while retaining the selected history duration
- Desktop shows a lightly softened live spectrum followed by its history, retaining distinct peaks and a common frequency axis
- Frequency scale, FFT size, smoothing, range, and spectral tilt controls
- Theme-colored ridges fading with age, or level-based heat colors
- Foreground ridges hide covered sections of older lines
- Available through the desktop add-scope menu and TUI layout editor (shortcut 8)
- Desktop popouts and saved profiles are supported; existing layouts stay unchanged
- Dedicated Prism Waterfall VST3/AU/CLAP plugin shares the desktop renderer and native history, with settings saved in DAW projects
- Hann-windowed FFT with 4× zero-padding
- Coherent amplitude normalization for calibrated spectral levels
- Native tests keep tone levels within 0.3 dB across multiple FFT sizes, amplitudes, and off-bin frequencies
- Logarithmic, Slaney Mel, and Linear frequency mapping
- Frequency placement is tested across 44.1, 48, and 96 kHz sample rates
- Classic mode provides a conventional spectral display
- Focused mode relocates local spectral peaks using phase correction and a local spectral centroid
- Sharp and Sharper perform phase-based frequency reassignment rather than post-process image sharpening
- Reassignment operates on every visible contributing FFT bin instead of only local maxima, preserving quieter partials and ambience
- Reassigned power compensates for Hann-window equivalent noise bandwidth and zero-padding so relocation remains level-calibrated
- Stereo analysis combines L/R energy rather than summing to mono, so anti-phase material remains visible instead of cancelling out
- Native tests verify reassigned tones stay on the correct Log, Mel, and Linear frequency rows
- Interactive inspection reports frequency, pitch, and time history
- FFT-based fundamental detection over a 2048-sample analysis window
- Pitch detector currently searches from 40 to 1000 Hz
- Pitch-lock dynamically retunes a narrow FIR band-pass around the detected fundamental
- Triggering follows a rising zero crossing rather than simply drawing the newest block of samples
- Trigger positions retain sub-sample precision
- Catmull-Rom interpolation is used when reading the waveform at fractional sample positions
- Adaptive pitch smoothing locks quickly at startup and becomes more conservative once stable
- Interactive measurement reports time, linear amplitude, and dBFS
- Full-band L/R analysis with no hidden high-frequency low-pass
- Native regression tests explicitly verify preservation of content above 8 kHz at 44.1, 48, and 96 kHz
- XY mode uses the original channel samples directly: Right on X, Left on Y
- XY and M/S Linear modes use calibrated channel-amplitude reference boundaries
- Polar retains an intentionally amplitude-compressed radial projection so low-level stereo structure remains readable
- Folded modes rotate negative-Mid samples rather than discarding them
- Adjustable display zoom from −12 to +24 dB without modifying the underlying signal
- Optional three-band stereo view with 250 Hz and 2.5 kHz crossovers
- Multiband analysis retains separate low, mid, and high L/R signals
- ITU-R BS.1770-style K-weighting using the pre-filter and RLB weighting stages
- Momentary loudness uses a 400 ms window
- Short-term loudness uses a 3 second window
- Integrated loudness uses overlapping 400 ms blocks with 100 ms hops
- −70 LUFS absolute gate
- Relative gate at −10 LU below ungated programme loudness
- Momentary, short-term, and integrated LUFS are calculated independently
- Stereo true-peak reconstruction uses a rate-aware 48-tap-per-phase FIR at 2× to 8× oversampling for common 44.1–192 kHz host rates
- Held L/R true-peak markers and a reset-scoped combined maximum are reported in dBTP
- 300 ms RMS integration window
- Adjustable 0 VU calibration from −30 to 0 dBFS
- Default reference is 0 VU = −14 dBFS
- Stereo correlation is calculated over the same analysis window and reported from −1 to +1
- 750 ms sample-peak hold
- Peak decay of 18 dB/s
- Bar envelope uses a 5 ms attack and 180 ms release
- Needle and bar displays can use the same underlying analysis
- Each rendered time column retains the minimum and maximum sample instead of selecting or averaging a single sample, helping preserve short transients while downsampling the history
- Mono and separate stereo-lane modes
- Optional multiband view calculates low, mid, and high RMS energy for every displayed time column
- Uses the same 250 Hz and 2.5 kHz multiband split as the vectorscope
- Interactive measurement reports time history, amplitude, and dBFS
- Native CoreAudio system-output capture on macOS using Audio Hardware Taps
- Native WASAPI loopback capture on Windows
- Native PulseAudio monitor-source capture on Linux
- Linux capture handles U8, 16-bit, 24-bit, 32-bit integer, and 32-bit floating-point PulseAudio formats before normalizing them for analysis
- Microphone and interface inputs use a separate low-latency AudioWorklet capture path
- Capture follows the active device sample rate instead of assuming a fixed 44.1 or 48 kHz analysis rate
- Keeps the previous 5, 10, 30, or 60 seconds of audio available without starting a recording beforehand
- Buffer retains 32-bit floating-point samples and exports standard RIFF/WAV files
- Mono and stereo capture are supported
- Choose 16-bit PCM (default) or 32-bit float WAV export in Rolling Capture settings; the choice is remembered across launches
- The export path supports source sample rates up to 384 kHz
- Captured audio can be dragged directly out of Prism as a file
- All eight Prism analyzers are built from the same native DSP source used by the desktop application
- Prism Bridge streams one DAW track or bus into the standalone app without changing the track audio
- VST3 and CLAP on Windows, macOS, and Linux
- AU on macOS
- Mono and stereo host layouts are supported
- Analyzer plugins are pure pass-through: Prism does not modify the host's audio buffer
- The realtime process callback only copies samples into a FIFO
- FFT, loudness, visualization, and other analysis work happens outside the realtime audio thread
- Scope configuration is serialized into the DAW's project/plugin state
- Plugins use JUCE 8 and a shared Prism web UI while keeping analysis native
- Native C++ frontend using the same Spectrum, Waterfall, Oscilloscope, Vectorscope, VU, Loudness, Spectrogram, Waveform, and system-capture implementations
- 60 FPS default rendering
- Experimental 120 FPS mode
- Compatibility mode uses 256-color output at up to 60 FPS
- Safe mode uses basic ANSI colors and caps rendering at 30 FPS
- Supports live output-device switching
- Supports input trim before every analyzer
- Includes pitch locking, vectorscope modes, calibrated VU reference levels, spectrogram reassignment modes, mono/stereo waveform views, and multiband analysis
- Reads Prism .iro themes and has its own shareable profile/customization system
- Typically uses around 35 MB of RAM
- Desktop visualizers can target 10, 30, 60, 120, or 144 FPS, or synchronize to the display refresh rate
- Spectrum, Spectrogram, Oscilloscope, and Waveform support interactive measurement overlays
- Measurement coordinates account for scope rotation and mirroring, so displayed readouts continue to correspond to the underlying signal after transforming a scope
- Linked Analysis maps only compatible semantic axes between scopes and hides guides when an exact value is outside the target's visible range
Prism can capture system output directly through CoreAudio on macOS, WASAPI on Windows, and PulseAudio on Linux. It can also switch to an input device when you want to analyze a microphone, interface, or line input.
No virtual audio cable is required for normal system capture.
The default rack measured around 7 ms median capture-to-render latency on an M5 Pro at 120 FPS.
The main rack and scope popouts can use solid, blurred, or clear backgrounds, making Prism usable as a normal desktop application or as a set of unobtrusive overlays.
Prism can also live in the system tray, start automatically with your computer, and launch either normally or out of the way when you want it running all the time.
Prism can continuously keep the last 5, 10, 30, or 60 seconds of audio in memory.
When you hear something you want to keep, drag the buffered audio out of Prism as a WAV file. There is no need to start recording beforehand.
Choose 16-bit PCM for smaller files or 32-bit float to preserve captured floating-point precision and samples above full scale for DAW editing. Changing the format applies to the next export without clearing buffered audio. Exports retain the source sample rate and do not normalize or dither audio.
The float buffer uses approximately 23 MB for 60 seconds of stereo at 48 kHz. Rolling Capture allocates no recorder buffer while off.
Every Prism scope is also available as a DAW plugin.
Drop a Spectrum, Oscilloscope, Vectorscope, Spectrogram, VU Meter, Loudness Meter, or Waveform onto a track and analyze it using the same interface and analysis engine as the desktop app.
- VST3 and CLAP on Windows, macOS, and Linux
- AU on macOS
- Settings are stored with your project
- Plugins follow your Prism themes and profiles
- Audio passes through untouched
Prism also installs Prism Bridge, a lightweight pass-through plugin for sending one DAW track or bus to the standalone application. Keep Prism open, insert Bridge on the source you want to inspect, then choose it under DAW Bridges in Prism's audio selector. Multiple Bridge instances can be available at once; only the one you select streams audio. Waveform and Spectrogram can optionally show host-derived Bars + Beats or Seconds rulers, including loop, seek, and packet-gap seams.
Bridge is available as VST3 and CLAP on Windows, macOS, and Linux and as AU on macOS. The AU is intentionally not marked sandbox-safe because it requires localhost access. Protocol details and host-validation notes are in docs/daw-bridge.md.
Existing VST3/AU versions have been tested in Ableton Live, FL Studio, and Reaper. CLAP requires a DAW that supports CLAP; see plugin build and validation notes.
The plugins ship alongside Prism. The Windows installer offers separate VST3 and CLAP checkboxes, both enabled by default. The macOS package installs VST3, AU, and CLAP; Linux deb/rpm packages install VST3 and CLAP. Archives support manual plugin installation; the Linux AppImage remains app-only. See installation instructions.
Prism also includes prism-tui, a native terminal interface built on the same capture and analysis code.
It provides real-time spectrum, metering, loudness, and other monitoring tools without needing to run the desktop interface.
prism-tui is lightweight, typically using around 35 MB of RAM.
prism-tui
prism-tui --list-outputs
prism-tui --output <id>
prism-tui --profile <name>
prism-tui --theme <name>
prism-tui --helpProfiles and .iro themes can be used from the TUI as well, and output devices can be changed without leaving it.
prism-tui --help lists the available controls and launch options.
A profile stores your Prism workspace: which scopes are visible, how they are laid out, their individual settings, and window state.
Keep different profiles for different setups or workflows and switch between them when needed.
Profiles are stored as .prsm files and can be shared with other Prism users.
Prism's interface is themeable through editable .iro files.
Themes control the colors used throughout the application and its scopes. You can edit your own, drop them into the Prism Themes folder, or download themes made by the community.
Prism also includes chroma-key-friendly themes for using scopes as overlays in OBS or other video software.
Prebuilt versions of Prism for Windows, macOS, and Linux are available on the Releases page.
Installable packages include the desktop application and the components supported by that package, including DAW plugins and prism-tui where applicable.
On Windows, the NSIS installer adds prism-tui to the machine PATH. Open a new terminal after installation so it inherits the updated environment. The portable Windows package does not modify PATH.
Prerequisites: Node.js 20.19+ or 22.12+ (Node 22.x is used in CI), npm, CMake 3.22+, and a C++ compiler toolchain.
| Platform | Toolchain |
|---|---|
| macOS | Xcode Command Line Tools |
| Windows | Visual Studio Build Tools |
| Linux | build-essential, python3, libasound2-dev, libpulse-dev, libgtk-3-dev, libwebkit2gtk-4.1-dev |
To build and test Linux from Windows using WSL2 or a Fedora VM over SSH, see
Linux testing. After setup, run npm run test:linux;
add -- --target fedora --suite full for Fedora plugin and package checks.
git clone https://github.com/Boof2015/prism.git
cd prism
npm installThe postinstall script compiles the native C++ module for your platform.
Use npm run rebuild:native to rebuild it for the installed Electron version
before running the desktop app. npm run build:native builds for your current
Node.js version, for example when running native tests directly with Node.
These commands select the project's node-gyp dependency explicitly to avoid
conflicts with the older copy bundled by Electron's build tools on Windows.
npm run dev # Development
npm run build # Build application assets
npm run configure:tui # Configure the standalone CMake project
npm run build:tui # Build prism-tui
npm run test:tui # Build and run native TUI tests
npm run build:plugins # Build bundled UI and native DAW plugins
npm run test:plugins # Build plugins and run native plugin tests
npm run install:plugins # Install built plugins (Windows prompts for UAC)
npm run test:lufsmeter-native # Run generated BS.1770/EBU true-peak vectors
npm run dist # Package for current platform
npm run dist:mac # macOS
npm run dist:win # Windows
npm run dist:linux # LinuxIf you have downloaded and extracted the official EBU Loudness Test Set for internal testing, run cases 15–23 without copying the WAVs into the repository. The files are not downloaded or redistributed by Prism, in accordance with the EBU test-sequence usage terms.
npm run test:lufsmeter-ebu -- /path/to/extracted-ebu-loudness-test-setThe TUI build downloads the pinned FTXUI source through CMake. Linux also requires the PulseAudio development package.
npm run build:plugins compiles the DAW plugins locally. npm run install:plugins copies the built files, requesting Windows UAC only for the protected copy; macOS/Linux default to user plugin folders. npm run dist builds and stages the complete plugin set before packaging on the current OS (the Linux AppImage remains app-only). See plugin/README.md for prerequisites and options.
Prism can optionally connect to Astra through its local API to show currently playing music, cover art, track information, and playback controls alongside your scopes.
Prism does not require Astra and works as a standalone application.
If you find Prism useful and want to support a broke college student, consider supporting development:
Prism is licensed under the GNU General Public License v3.0. See LICENSE for the full text.
Third-party license notices are recorded in THIRD_PARTY_NOTICES.md.