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Acoustical measurements in a 1:10 scale model of a multi-purpose hall

Identifieur interne : 000170 ( PascalFrancis/Curation ); précédent : 000169; suivant : 000171

Acoustical measurements in a 1:10 scale model of a multi-purpose hall

Auteurs : Jin Yong Jeon [Corée du Sud] ; Jong Kwan Ryu [Corée du Sud]

Source :

RBID : Pascal:04-0182920

Descripteurs français

English descriptors

Abstract

Measurements were made in a 1:10 scale model of a 1500-seat multi-purpose hall to investigate the acoustic properties of its opera mode. The length from the stage front to the rear wall is 33 m and its maximum width is 28 m with a volume of 14300 m3. Reflecting surfaces were included to scatter early energy from the stage area onto the audience areas. Several settings of the sources were used on the platform and in the pit in order to determine how a lack of brilliance caused by diffraction occurred in the stalls audience. The advantages of the curved ceiling surface in front of the proscenium above the orchestra pit were exploited. In addition, the effect of some diffusing treatments on surfaces adjacent to the pit and on the side walls was also investigated.
pA  
A01 01  1    @0 0001-4966
A02 01      @0 JASMAN
A03   1    @0 J. Acoust. Soc. Am.
A05       @2 115
A06       @2 5
A08 01  1  ENG  @1 Acoustical measurements in a 1:10 scale model of a multi-purpose hall
A11 01  1    @1 JEON (Jin Yong)
A11 02  1    @1 RYU (Jong Kwan)
A14 01      @1 School of Architectural Eng., Hanyang Univ., Seoul 133-791, Korea @Z 1 aut. @Z 2 aut.
A20       @2 p. 2476
A21       @1 2001-05-04
A23 01      @0 ENG
A43 01      @1 INIST @2 129
A44       @0 8100 @1 © 2004 American Institute of Physics. All rights reserved.
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A61       @0 A
A64 01  1    @0 The Journal of the Acoustical Society of America
A66 01      @0 USA
C01 01    ENG  @0 Measurements were made in a 1:10 scale model of a 1500-seat multi-purpose hall to investigate the acoustic properties of its opera mode. The length from the stage front to the rear wall is 33 m and its maximum width is 28 m with a volume of 14300 m3. Reflecting surfaces were included to scatter early energy from the stage area onto the audience areas. Several settings of the sources were used on the platform and in the pit in order to determine how a lack of brilliance caused by diffraction occurred in the stalls audience. The advantages of the curved ceiling surface in front of the proscenium above the orchestra pit were exploited. In addition, the effect of some diffusing treatments on surfaces adjacent to the pit and on the side walls was also investigated.
C02 01  X    @0 001B40C55
C03 01  3  FRE  @0 4355F @2 PAC @4 INC
C03 02  3  FRE  @0 Etude expérimentale
C03 02  3  ENG  @0 Experimental study
C03 03  3  FRE  @0 Etude théorique
C03 03  3  ENG  @0 Theoretical study
N21       @1 124
N47 01  1    @0 0416M000895

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Pascal:04-0182920

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