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№1 слайд
The importance of the direct
Содержание слайда: The importance of the direct to reverberant ratio in the perception of distance, localization, clarity, and envelopment David Griesinger Consultant Cambridge MA USA www.DavidGriesinger.com

№2 слайд
Introduction Sound engineers
Содержание слайда: Introduction Sound engineers need (almost) no convincing about the importance of direct sound. The sound image in most popular recordings is built from close-miked sources. Reverberation is added later as an enhancement, the sauce that holds the sound together. There is a fiction among classical engineers that the “hauptmicrophone” picks up the direct sound But in practice the image is created by accents, and the main mike adds some early reflections. My research into spatial acoustics started with sound recording, and the hall research of Michael Barron.

№3 слайд
Barron s Spatial Impression
Содержание слайда: Barron’s Spatial Impression Diagram

№4 слайд
My research I used a similar
Содержание слайда: My research I used a similar setup, but employed six or more reflections at various angles and delays. I obtained similar results – and found it was the total energy of the delays that mattered, not the amplitude of the individual reflections. The theory of how the ear detects such reflections in the presence of music followed, with many interesting results. But the range of the energy of the reflections was the same as Barron’s – about -25dB to +5dB with respect to the direct. In this talk I will refer to the Direct to Reverberant ratio (D/R). In terms of D/R, Barron’s range is +25dB to -5dB.

№5 слайд
Results for D R dB to dB Dry
Содержание слайда: Results for D/R=+25dB to 0dB Dry speech Note the sound is uncomfortably close Mix of dry with early reflections at -5dB. (D/R = +5dB) The mix has distance (depth), and is not muddy! Note there is no apparent reverberation, just depth. Same but with the reflections delayed 20ms at -5dB. (+5dB D/R) Note also that with the additional delay the reflections begin to be heard as discrete echos. But the apparent distance remains the same. Same but with the reflections delayed 50ms at -3dB (+3dB D/R) Now the sound is becoming garbled. These reflections are undesirable! If the speech were faster it would be difficult to understand. Same but with reflections delayed 150ms at -12dB (+12dB D/R) I also added a few reflections between 20 and 80ms at a level of -8dB to smooth the decay. Note the strong hall sense, and the lack of muddiness. Note the Late reflections are at least 7dB more audible than the early ones!!! And the sense of hall is all in the late reflections!!!

№6 слайд
Preference and Practice In
Содержание слайда: Preference and Practice In recording practice the D/R for the combination of early and late reflections is nearly always between +4 and +6dB If you give an engineer a control which varies D/R, and ask them to set an optimum value, this is what they choose. Acousticians (including Beranek) choose the same values. Regardless of the material, reverberation in reproduced music should be strong enough to be audible, And weak enough not to reduce intelligibility or clarity These values of D/R are optimums based on human hearing and the properties of music. Otherwise engineers, producers, conductors and musicians would insist on something else. But these are NOT the values of D/R found in halls!

№7 слайд
Concert Halls Barron was
Содержание слайда: Concert Halls Barron was interested in halls, not recordings! The critical distance in Boston Symphony Hall (BSH) is ~ 7meters. At this distance the D/R is 0dB. Almost all the listeners are beyond this distance. The average D/R is below -8dB. In halls the majority of the loudness is in the reflections Otherwise the music would not be loud enough throughout the hall. When we experiment with D/R values less than 0 very different results emerge. And the results have large – and controversial – implications for hall design.

№8 слайд
Experiences Staatsoper Berlin
Содержание слайда: Experiences – Staatsoper Berlin

№9 слайд
Experiences Bolshoi a
Содержание слайда: Experiences – Bolshoi – a famously good hall for opera

№10 слайд
New Bolshoi before
Содержание слайда: New Bolshoi before modification

№11 слайд
Experiences Amsterdam
Содержание слайда: Experiences – Amsterdam Muziektheater Peter Lockwood and I spent hours adjusting the reverberant level using a remote in the hall. He taught me to hear the point where the direct sound becomes no longer perceptible, and the sonic distance dramatically increases. With a 1/2 dB increase in reverberant level, the singer moved back 3-4 meters. In Copenhagen, I once decreased the D/R by one dB while Michael Schonwandt was conducting a rehearsal. He immediately waved to me from the pit, and told me to put it back. Given a chance to listen A/B, these conductors choose dramatic intensity over reverberance. When they do not have this chance, reverberation is seductive, and the singers be damned!

№12 слайд
Experiences, Copenhagen New
Содержание слайда: Experiences, Copenhagen New Stage

№13 слайд
INVOLVEMENT, not ENVELOPMENT
Содержание слайда: INVOLVEMENT, not ENVELOPMENT All these experiences relate to the importance of the perception of direct sound in drama and opera. I believe the same is true of music. At the IOA conference in Oslo, Krokstad gave a lecture where he insisted that acousticians needed to provide involvement, not envelopment And not just for drama and opera, but for chamber music and symphony too. At the end of the lecture he showed a picture of the Theatre de Colon in Brazil. “Is this the concert hall of the future” he asked? It is the independent perception of the direct sound that involvement requires We must learn how to provide this essential element in halls. I was recently fortunate to hear the Metropolitan Opera performance of Salome in HD at a good theater. The sound was harsh and dry – but you could hear every syllable of a fabulous performance. This is the dramatic and sonic experience the audience will increasingly come to demand.

№14 слайд
Main Points The ability to
Содержание слайда: Main Points The ability to hear the Direct Sound – the sound energy that travels to the listener without reflecting – is a vital component of the sound quality in a great hall. The ability to separately perceive the direct sound when the D/R is less than 0dB requires time. There must be sufficient time between the arrival of the direct sound and the build-up of the reverberation Hall shape does not scale Our ability to perceive the direct sound depends on its level compared to reflected sound, and on the time-gap between the two. Both the direct to reverberant ratio (d/r) and the time-gap change as the hall size scales – but human hearing (and the properties of music) do not change. A hall shape that provides great sound to a high percentage of 2000 seats may produce a much lower percentage of great seats if it is scaled to 1000.

№15 слайд
Main Points Current acoustic
Содержание слайда: Main Points 2 Current acoustic measures ignore both the D/R and the time gap between the direct (the first wavefront) and the reverberation. RT, C80, and EDT all ignore the strength of the direct sound, and the effects of musical style on the audibility of the D/R The strength of the reverberation depends on the length of a note compared to the reverberation time. Short sounds do not excite a large hall, and the D/R in practice can be much higher than expected from conventional theory. There need to be gaps between notes sufficiently long that the reverberance decays below the level of the new direct sound. The direct sound from notes that differ in pitch by at least a musical fifth are easier to distinguish. We need measures that use binaural recordings of actual performances as inputs. And the ability to listen to these recordings to test the validity of these measures against the true experience. Two such measures will be discussed here. Methods for accurately making and reproducing binaural recordings are discussed in another paper.

№16 слайд
Diffusing elements do not
Содержание слайда: Diffusing elements do not scale The audibility of direct sound is frequency dependent. Frequencies above 1000Hz are particularly important Diffusing elements can cause the D/R to also vary with frequency in ways that improve direct sound audibility. The best halls (Boston, Amsterdam, Vienna) all have ceiling and side wall elements with box shape and a depth of ~0.4m. These elements tend to send frequencies above 1000Hz back toward the orchestra and the floor, where they are absorbed. The result is a lower early and late reverberant level above 1000Hz in the rear of the hall. This increases the D/R for the rear seats, and improves clarity. Replacing these elements with smooth curves or with smaller size features does not achieve the same result. Some evidence of this effect can be seen in IACC80 measurements when the hall and stage are occupied.

№17 слайд
Sound Build-up in halls, or
Содержание слайда: Sound Build-up in halls, or why do different large halls sound different? In a large hall – such as Boston Symphony (BSH), or the Amsterdam Concertgebouw (CG) the reverberation decay is nearly identical, but the halls sound different. I decided to examine the way reverberation builds up compared to the direct sound, instead of the way it decays. I used a simple binaural image-source model with HRTFs measured from my own eardrums.

№18 слайд
Reverberation build-up and
Содержание слайда: Reverberation build-up and decay – from models

№19 слайд
Smaller halls What if we
Содержание слайда: Smaller halls What if we build a hall with the shape of BSH, but half the size? The new hall will hold about 600 seats. The RT will be half, or about 1 second. We would expect the average D/R to be the same. Is it? How does the new hall sound? If the client specifies a 1.7s RT will this make the new hall better, or worse?

№20 слайд
Half-Size Boston
Содержание слайда: Half-Size Boston

№21 слайд
An existing small hall
Содержание слайда: An existing small hall

№22 слайд
An existing small hall -
Содержание слайда: An existing small hall - pictures

№23 слайд
Small shoebox halls can be OK
Содержание слайда: Small shoebox halls can be OK If the client insists on a shoebox it can work by building a large hall and installing a small number of seats. I was just in such a small hall in Helsinki, and at least half the seats were OK. But this is not the ideal solution. With a different shape nearly all the seats could have been OK – and it might have been less expensive.

№24 слайд
Great Small Halls Exist!
Содержание слайда: Great Small Halls Exist!

№25 слайд
Williams Hall, NEC Williams
Содержание слайда: Williams Hall, NEC Williams hall, in the same building, has ~350 seats in a square plan with a high ceiling. Once again the sound is clear and reverberant in most, if not all, seats.

№26 слайд
Hard learned lessons Where
Содержание слайда: Hard learned lessons Where clarity is a problem in small halls, acousticians usually recommend adding early reflections – through a stage shell, side reflectors, etc. These measures reduce the gap between the direct sound and the reflected energy They increase the sense of distance to the performers, and the muddiness. They also increase loudness, which is almost always too high already A better way is to add absorption, or perhaps diffusion, to reduce the level of the earliest reflections. Small halls have strong direct sound and too many early reflections The reflections also come too quickly Adding more reflections is exactly the wrong thing to do. Adding absorption will improve clarity but reduce the late reverberant level and the RT. Electronics, or more cubic volume, can restore the longer RT without decreasing the D/R Adding absorption is NOT recommended unless the decrease in late reverberation can be compensated. If electronics are used they must be on all the time.

№27 слайд
Clarity and involvement come
Содержание слайда: Clarity and involvement come from the direct sound. Spaciousness and envelopment are provided by LATE energy. Reflections in the time range of 50 to 100ms can increase loudness – but tend to reduce clarity and intelligibility. Reflections from 20 to 50ms can increase intelligibility – but they decrease involvement. A few Early lateral reflections can help blend together the orchestra image, but they do not provide significant envelopment. When the direct sound is adequate for localization, and there is lots of late reverberation, the spatial perception of early reflections is inhibited. You can often make the reflections in the time range of 20ms to 80ms monaural with no change in sound. A hall with good reverberance will emphasize late reverberation over early reflections And ideally it should provide a lower level of reverberation above 1000Hz in the back of the hall. This will provide loudness and clarity to the largest number of seats.

№28 слайд
Why do current acousticians
Содержание слайда: Why do current acousticians emphasize early reflections? I believe the current emphasis on early reflections (which include reflections in the deadly range of 50-80ms) is a result of a mis-application of Barron’s data for D/R greater than 0dB. When D/R is below 0dB we find that it is the spatial properties of the late reverberation that dominate perception. The correlation between hall quality and “early time delay gap” found by Leo Beranek applies only to large halls. In a large hall excessive width can lead to disturbing echoes in some seats. Leo told me his interest in the subject started when he was working in such a hall. Our work shows that there may be an optimum delay gap. The ~ 25 ms observed in BSH may be close to that optimum. The Amsterdam hall, which is both clearer and more reverberant, sometimes has echoes – particularly on solo piano. The Musikverrein in Vienna has a shorter gap, and a longer RT than BSH. Seats in the rear half of the hall sound muddy and distant to this author. Best to sell them to tourists… The standing room (under the balcony) is surprisingly good!

№29 слайд
Threshold Data Onset and
Содержание слайда: Threshold Data Onset and azimuth thresholds allow hall sound to be predicted from models! 1. Thresholds for azimuth detection. Azimuth experiments are simple, and repeatable. 2. Thresholds for onset enhancement Onset enhancement is also easy to quantify. 3. Thresholds for elevation detection. Work is on-going. Accurate HRTFs are needed in models 4. Thresholds for diffuse field detection Also depends on accurate HRTFs We have a data set of HRTFs from a precise model of a single individual, including the ear canal and eardrum impedance. This data is available for the asking…

№30 слайд
Experiment for threshold of
Содержание слайда: Experiment for threshold of Azimuth Detection in halls

№31 слайд
Threshold for azimuth
Содержание слайда: Threshold for azimuth detection as a function of T10

№32 слайд
An important caveat! All
Содержание слайда: An important caveat! All these thresholds were measured without visual cues The author has found that in a concert (with occasional visual input) instruments (such as a string quartet) are perceived as clearly localized and spread. When I record the sound with probes at my own eardrums, and play it back through calibrated earphones the sound seems highly accurate, but localization often disappears! Without visual cues when the d/r is below threshold the individual instruments are localized and spread when they play solo, but collapse to the center when they play together. My brain will not allow me to detect this collapse when I am in the concert hall – even if I close my eyes most of the time! With eyes closed it is more difficult to separate the sounds of the individuals, such as the second violin and the viola. This difficulty persists in the binaural recording.

№33 слайд
How to use the Thresholds
Содержание слайда: How to use the Thresholds These thresholds provide guidelines for hall design. As a first approximation the d/r value can come directly from classical acoustics, where for typical hall absorption and an RT of 2s: d/r ~= 20*log10(0.14*sqrt(R)/d_source) + d_source/30 Where: R = room constant = S*a_av/(1-a_av) S = total surface area d_source = source distance in ft a_av = average absorption coefficient d/r scales with hall dimensions as long as the source to listener distance decreases linearly with the sqrt of the area. (And the music uses shorter notes by the same factor!) But the time gap decreases – and if a_av is reduced to keep RT constant, than d/r will decreases also. The net result is that localization decreases in small halls unless the shape is changed.

№34 слайд
In practice the D R is
Содержание слайда: In practice the D/R is different than expected from classical acoustics The D/R is frequency dependent in halls, and the D/R above 1000Hz is critically important for the detection of direct sound and musical involvement. Surface features can be used to increase D/R at higher frequencies. In addition, the distribution of absorption in a hall significantly alters the distribution of the D/R. A high ceiling with a lot of reflecting surfaces above the audience can increase RT without reducing the average D/R, because there is less excitation of the more distant volume, and the reverberation created tends to stay up high. Effort should be to keep the D/R above ~700Hz as constant as possible over the maximum number of seats. Current modeling techniques may not properly calculate these effects. Old fashioned light models might work better…

№35 слайд
Light models
Содержание слайда: Light models

№36 слайд
Modeling T Classical
Содержание слайда: Modeling T10 Classical acoustics predicts a starting value for d/r. We can make a chart of d/r values in all the seats of a proposed hall. T10 does not follow easily from classical acoustics, but can be predicted with fair accuracy with a simple computer model of the hall. Just the basic hall dimensions are needed. From this data we can predict the localizability of sound in all the seats. The results can be surprising! Auralization from these models (given accurate HRTFs) can be convincing.

№37 слайд
Onset Enhancement
Содержание слайда: Onset Enhancement

№38 слайд
Small Hall Shapes
Содержание слайда: Small Hall Shapes

№39 слайд
Retro reflectors above Hz
Содержание слайда: Retro reflectors above 1000Hz

№40 слайд
High frequency retro
Содержание слайда: High frequency retro reflectors

№41 слайд
High frequency overhead
Содержание слайда: High frequency overhead filters

№42 слайд
Binaural Measures
Содержание слайда: Binaural Measures

№43 слайд
Localization
Содержание слайда: Localization

№44 слайд
Localization surface
Содержание слайда: Localization – surface1

№45 слайд
Localization, Surface
Содержание слайда: Localization, Surface 2

№46 слайд
Localization a poor seat
Содержание слайда: Localization – a poor seat

№47 слайд
Measures based on harmonic
Содержание слайда: Measures based on harmonic coherence When the formant frequencies above 1000Hz are disturbed by reflections, the phase relationship between harmonics of solo instruments is randomized. The result is highly audible, and is a primary cue for the distance of an actor, singer, or soloist. The perception has been described by Zwicker as “roughness”. This effect can be easily measured, and is sensitive both to medial and lateral reflections.

№48 слайд
Another singer
Содержание слайда: Another singer

№49 слайд
Some demos of eardrum
Содержание слайда: Some demos of eardrum recordings These recordings have been equalized for loudspeaker reproduction. You may be able to judge clarity and intelligibility over near-field loudspeakers. Accurate headphone reproduction requires headphone equalization If probes are available the method described here will work, A method which uses equal loudness curves will be described later in this paper. opera balcony 2, seat 11 Moderate intelligibility, reverberant sound. OK for non-Italian speakers with subtitles opera balcony 3, seat 12 Poor intelligibility, very reverberant opera standing room Deep under balcony 2 – good intelligibility This was preferred by Italian speakers A concert hall – row 8 (quite close) Very good sound. Not so good further back.

№50 слайд
Conclusions Performance
Содержание слайда: Conclusions Performance venues should maximize involvement, not envelopment To achieve this goal the direct sound must be perceived by the brain as distinct from the reflected energy – and this includes early reflections from all directions. The optimum value for the d/r ratio depends on the hall size – The D/R ratio must increase as hall size is reduced if clarity is to be maintained. D/R can be increased by decreasing the average seating distance, decreasing the reverberation time, increasing the hall volume, or by careful use of rectangular diffusing elements. This is particularly true in opera houses and halls designed for chamber music. A 1.8 second reverberation time is NOT necessarily ideal in a 1000 seat hall!!! Remember that changes in reverberant LEVEL (D/R) are far more audible than changes in RT. To maintain clarity, low sonic distance, and azimuth detection in a small hall it is desirable to reduce the average seating distance, and widely diffuse or absorb the earliest reflections, whether lateral or not. The best small halls do this already. Current hall measurements ignore both the D/R and the time gap between direct and reverberation. Better measures exist. They must be used if the current practice of hall design is to be improved.

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