--- license: cc-by-4.0 task_categories: - audio-classification tags: - audio - noise - rir - augmentation - dns-challenge - microphone - impulse-response pretty_name: DNS Noise + RIR (24k mono) configs: - config_name: default data_files: - split: noise path: noise/*.parquet - split: rir path: rir/*.parquet - split: mic_ir path: mic_ir/*.parquet --- # DNS-Noise DNS-Challenge `noise_fullband` and `impulse_responses` republished as 24 kHz mono FLAC for on-demand streaming augmentation, plus a microphone-characteristics split. Three splits: - `noise` — environmental noise (long files segmented into chunks) - `rir` — room impulse responses (one row per file) - `mic_ir` — microphone impulse responses (one row per file) ```python from datasets import load_dataset noise = load_dataset("ChristianYang/DNS-Noise", split="noise", streaming=True) rir = load_dataset("ChristianYang/DNS-Noise", split="rir", streaming=True) mic_ir = load_dataset("ChristianYang/DNS-Noise", split="mic_ir", streaming=True) ``` ## mic_ir split Microphone impulse responses for simulating microphone frequency colouration, aggregated from three sources. `source_file` is prefixed with the source dataset: | prefix | source | content | |---|---|---| | `madir/` | [Zenodo 4633508](https://zenodo.org/records/4633508) — Multi-Angle, Multi-Distance Microphone Impulse Response Dataset (CC-BY-4.0) | studio mics, `Raw_IRs` only, one bit-depth variant per IR (24-bit preferred); folder names encode mic model, polar pattern, distance and angle | | `micirp/` | [MicIRP](http://micirp.blogspot.com) via [audb](https://github.com/audeering/audb) v1.0.0 (CC BY-SA 4.0) | vintage/classic microphones | | `ctf_2020_tiny_irs/` | Collected Transients "Tiny IRs" (2020) | consumer-device microphone captures (cellphone/tablet/laptop/camera mics, incl. mic-through-speaker chains); pure loudspeaker IRs are excluded | Processing: mixed down to mono, resampled to 24 kHz (soxr HQ), peak-normalised to 0.97, encoded as 16-bit FLAC. Absolute level is not meaningful — normalise IR energy before convolution.