Line Array Systems across India

A line array is a coverage engineering exercise, not a stack of boxes. We model the room or the ground in prediction software — Soundvision for L-Acoustics, ArrayCalc for d&b — using the actual seating geometry, trim height and surface materials. The output is a splay-angle schedule for each box in the hang, a rigging plot with point loads, and an SPL map that shows what the last row receives against the front row. The design target for speech-heavy and large-crowd work is coverage within about ±3 dB across the audience, with energy deliberately kept off ceilings, rear walls and any surface that returns a late reflection.

Distance is solved with time, not volume. Beyond roughly 50 to 60 metres the direct sound from the main hang has lost too much level and high frequency to carry intelligibility, so we add delay positions. Each one is timed against the measured distance from the main array at the local speed of sound — about 2.9 milliseconds per metre, adjusted for air temperature, which moves measurably across a hot afternoon into a cool night. We usually add one to three milliseconds of extra delay so the main system still arrives first and the audience localises the stage rather than the tower beside them.

Subwoofers get their own geometry. An end-fire or cardioid sub array cancels rearward energy, which keeps low frequency off the stage, out of the microphones and away from the nearest residential boundary — often the single most useful thing we can do for a noise condition. Amplification is specified with redundancy at the rack level, dual supply feeds where the site allows, and a network topology that survives a cut cable. Final alignment is measured with Smaart at multiple positions in the audience, not set from a factory preset, and the measured traces are part of the handover documentation.