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Dynamic higher-order stereophony

Dynamic higher-order stereophony
Dynamic higher-order stereophony

Higher-Order Stereophony is a new spatial audio approach which extends classic stereo to higher order soundfield reproduction and generalised loudspeaker arrays, in a similar manner to Higher-Order Ambisonics. Higher-Order Stereophony reproduces the soundfield accurately across a line only, which must be orientated to align with the listener's interaural axis. This work introduces Dynamic Higher-Order Stereophony, which expands the technique to include listener tracking using dynamic amplitude panning. This means the soundfield is reproduced across a dynamically moving line dependent on the listener's orientation, to ensure correct reproduction of a desired set of binaural signals. A number of classic stereo approaches are shown to be special cases of first order Stereophony, and decoders to reproduce Higher-Order Ambisonics content using the new technique presented. A listening test comparing Higher-Order Stereophony and Ambisonics reproduction, low-passed at 4 kHz to reduce spatial aliasing artefacts, shows that the former technique can perform equally well as Ambisonics to the same truncation order with respect to positional properties of a virtual sound source, while using a smaller number of loudspeakers. The approach can also produce rear virtual sources using only loudspeakers positioned in the front of the listener, however with the requirement of listener tracking.

Spatial audio, higher-order ambisonics (HOA), higher-order stereophony (HOS), panning, stereophony
2329-9304
2073-2084
Hollebon, Jacob
75e4dd71-cfb5-4d28-82a5-7ee1bee73207
Fazi, Filippo Maria
Hollebon, Jacob
75e4dd71-cfb5-4d28-82a5-7ee1bee73207
Fazi, Filippo Maria

Hollebon, Jacob and Fazi, Filippo Maria (2024) Dynamic higher-order stereophony. IEEE/ACM Transactions on Audio, Speech, and Language Processing, 32, 2073-2084. (doi:10.1109/TASLP.2024.3379878).

Record type: Article

Abstract

Higher-Order Stereophony is a new spatial audio approach which extends classic stereo to higher order soundfield reproduction and generalised loudspeaker arrays, in a similar manner to Higher-Order Ambisonics. Higher-Order Stereophony reproduces the soundfield accurately across a line only, which must be orientated to align with the listener's interaural axis. This work introduces Dynamic Higher-Order Stereophony, which expands the technique to include listener tracking using dynamic amplitude panning. This means the soundfield is reproduced across a dynamically moving line dependent on the listener's orientation, to ensure correct reproduction of a desired set of binaural signals. A number of classic stereo approaches are shown to be special cases of first order Stereophony, and decoders to reproduce Higher-Order Ambisonics content using the new technique presented. A listening test comparing Higher-Order Stereophony and Ambisonics reproduction, low-passed at 4 kHz to reduce spatial aliasing artefacts, shows that the former technique can perform equally well as Ambisonics to the same truncation order with respect to positional properties of a virtual sound source, while using a smaller number of loudspeakers. The approach can also produce rear virtual sources using only loudspeakers positioned in the front of the listener, however with the requirement of listener tracking.

Text
Dynamic Higher Order Stereophony - Accepted Manuscript
Available under License Creative Commons Attribution.
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More information

Accepted/In Press date: 4 March 2024
e-pub ahead of print date: 27 March 2024
Published date: 27 March 2024
Additional Information: Publisher Copyright: © 2014 IEEE.
Keywords: Spatial audio, higher-order ambisonics (HOA), higher-order stereophony (HOS), panning, stereophony

Identifiers

Local EPrints ID: 490490
URI: http://eprints.soton.ac.uk/id/eprint/490490
ISSN: 2329-9304
PURE UUID: 6d909620-936f-43db-a5a0-986a104cb23c
ORCID for Jacob Hollebon: ORCID iD orcid.org/0000-0002-4119-4070

Catalogue record

Date deposited: 28 May 2024 17:08
Last modified: 11 Jun 2024 02:02

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Contributors

Author: Jacob Hollebon ORCID iD
Author: Filippo Maria Fazi

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