Spatial audio's progression from delta stereophony to techniques like DBAP, VBAP, MDAP, and Ambisonic panning, also including Wave Field Synthesis (WFS) with its extensive multi-loudspeaker arrays, has focused on achieving precise spatialization over large listening areas. This listening experiment evaluates localization errors and apparent source width of audio objects rendered with NESS algorithm (distance-based amplitude and delay panning) within a 200-seat amphitheatre. Factors such as loudspeaker setup, source and listener positions, and audio stimulus types were analysed. Results indicate a strong correlation between perceived and predicted source directions using the extended energy vector model; however, the model's predictions for apparent source width were less consistent. These outcomes highlight the model's utility and suggest further refinement for source width estimation.
Authors:
Jacquet, Damien; Dominguez, Johana; Petiot, Jean-François
Affiliations:
Arbane Groupe, Bouguenais, France; Ecole Centrale de Nantes, LS2N, UMR CNRS 6004, 44321 Nantes, Franc; Arbane Groupe, Bouguenais, France(See document for exact affiliation information.)
AES Conference:
AES 2024 International Conference on Acoustics & Sound Reinforcement (January 2024)
Paper Number:
15
Publication Date:
January 23, 2024
Subject:
Acoustics & Sound Reinforcment
Click to purchase paper as a non-member or you can login as an AES member to see more options.
No AES members have commented on this paper yet.
To be notified of new comments on this paper you can subscribe to this RSS feed. Forum users should login to see additional options.
If you are not yet an AES member and have something important to say about this paper then we urge you to join the AES today and make your voice heard. You can join online today by clicking here.