WHAT DOES YOUR SOUND LOOK LIKE?A COMMUNITY IN THE MAKING

YOUR SOUND.
MADE VISIBLE.

Sing or hum a steady note and watch your voice shape the field.

Your voice stays on your device.We don’t record, upload, store, or keep your voice sample.

MICROPHONE OFF

Microphone off. The field shows a demonstration response.

A magnified virtual water surface responds to your detected frequency. Reflected light reveals its ripples, shown in slow motion. Your detected note is also available as text.

A future community
for people who make music.

WHY DOES THE PATTERN CHANGE?

A note. A ripple. A response.

Your pitch sets the driving frequency. Gravity and surface tension shape how this water moves. Some frequencies excite stronger resonances; others bring different modes into play.

This is the modeled response of one defined water surface, driven by your fundamental pitch rather than your voice’s full spectrum. Change its size, depth, or boundary and the same note can produce a different pattern.

From voice to visible.

  1. Voice Analyzed only on your device
  2. Frequency YIN pitch detection · A4 = 440 Hz · approximately 65–1,200 Hz
  3. Water model Gravity + surface tension + resonant modes
  4. Response Ripples revealed by reflected light
THE SURFACE, DEFINED

A magnified, circular water well in a rigid surface: 6 mm across and 1 mm deep. Water at approximately 20°C: density 998 kg/m³, surface tension 0.0728 N/m, kinematic viscosity 1.004 × 10⁻⁶ m²/s; gravity 9.81 m/s². The idealized wall and bottom are impermeable. The contact line moves freely with a 90° contact angle and zero radial surface slope.

We use linear, small-amplitude capillary–gravity modes: Jₘ(αr/R) cos[m(θ−θ₀)], with J′ₘ(α) = 0 and k = α/R. Their natural frequencies satisfy ω² = (gk + γk³/ρ) tanh(kh). The complex response sums 70 modes: angular orders 0–9 and seven nonzero radial roots each. The uniform mode is excluded to conserve water volume.

Your measured pitch drives an idealized harmonic point-pressure force at 0.39 of the radius and angle 0.35 radians. Modal decay is approximated by β = 2νk² + 0.012ωₙ; response denominators are ωₙ² − ω² + 2iβω. This damping is not calibrated to a real vessel. The model omits detailed wall losses, nonlinear waves, splashes, and vertically driven Faraday instabilities. It does not simulate how your voice would transmit force into a real pool.

The water is magnified, its response normalized, and visible slopes enhanced. Fine lines trace equal-response levels at 10%, 24%, and 46% of the peak displacement amplitude; they are explanatory contours, not permanent nodes or light emitted by water. Broad lighting makes the full response visible, including at lower pitches. Motion plays in illustrative slow motion (approximately 0.27 cycles per second during input and 0.09 while idle) so the ripples can be seen; the actual detected frequency still determines the spatial response. Reflections, shadows, and edge highlights are artistic lighting, not measured optical effects. Transitions blend steady-state responses; this is not a transient fluid solver or a validated laboratory simulation. Finite mode and rendering resolution limit precision.

Before microphone use, the idle field uses a fixed 220 Hz demonstration input. While listening, silence or an uncertain pitch gently returns the field toward the demonstration response. Stop Microphone releases access and holds the last pattern. Sing a steady note to drive the model again. No microphone data is used until you activate it. Your audio is never uploaded or stored.

Water-wave dispersion · MIT
Contact-line and damping assumptions · Bongarzone & Gallaire
YIN pitch estimator · de Cheveigné & Kawahara

01 / THE REASONA COMMUNITY IN DEVELOPMENT

SOME THINGS
YOU CAN’T
MAKE ALONE.

The part you hear
but can’t play.

A voice for your track. A drummer for your band. Someone who hears where you’re trying to go.

I Make Music is being built to help people who make music find each other. To share the work, learn from each other, and make something together.

Bring your sound.
Find what’s possible.

BE HERE AT THE BEGINNING ↗

Musicians. Singers. Producers. Songwriters. Composers. Teachers. Students. Bands. Creators.

02 / WHAT’S COMINGPLANNED. NOT LIVE YET.

THE NEXT
PART IS PEOPLE.

The vision is taking shape.
These are the connections we’re building toward. Features are planned and may evolve.

01

SHOW WHAT
YOU MAKE.

PROFILES + SHARE

Your instruments. Your interests. Your work. Build a musical identity with your bio, genres, skills, goals, music, and YouTube videos.

COMING SOON
02

FIND YOUR
PEOPLE.

DISCOVER + CONNECT + MESSAGE

Search by instrument, genre, location, skills, interests, and creative goals. Find people nearby or available remotely. Build connections and, in time, message privately.

COMING SOON
03

MAKE IT
TOGETHER.

COLLABORATE

Find band members, vocalists, songwriters, producers, and session musicians. Make something locally or across a distance.

COMING SOON
04

LEARN.
PASS IT ON.

LEARN + TEACH

Find a teacher. Develop your sound. Share what you know through free or paid lessons.

COMING SOON
05

PUT YOUR
NAME ON IT.

MERCH

Planned print-on-demand tools for musicians. Turn the identity you’re building into merchandise of your own.

COMING SOON

03 / THE FIRST WAVE

BE HERE
AT THE
BEGINNING.

We’re building a place for people who make music. People like you.

Join the early list for launch updates and to hear when profiles open.

Your next collaboration has to start somewhere.

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