Far Wide Radio

Far Wide Radio translates telescope data into sound. Each programme works from a single James Webb Space Telescope (JWST) or Dark Energy Spectroscopic Instrument (DESI) spectral cube, read directly by custom-made algorithms — no illustration, no mood music laid over a picture. Four instruments make the series. A batch engine sonifies a chosen field of the data — brightness, gradient, boundary, obstruction, lines, flow, holonomy, anisotropy — on a fixed bench: image row becomes pitch, column becomes stereo position, wavelength becomes time. Sometimes these are rendered clean of the continuum the telescope sends with the signal; sometimes it is kept, for its harmonic effect. A spectral voice inverts that bench: wavelength becomes pitch rather than time, flux becomes loudness, and redshift becomes a downward transposition — so the further back the light comes from, the lower it falls. A sheaves-based motif finder selects passages by the rarity and uniqueness