----- Build your last loudspeakers yourself -----

 

 

What's new

 

Concepts

Stereo Recording and Rendering

Audio production

Loudspeakers

Crossovers

Room acoustics

Issues in 
speaker design

 

 

Projects

LXmini

LX521
reference

ORION
challenge

ORION-3.4

PLUTO-2.1

WATSON-SEL

PLUTO+
subwoofer

THOR
subwoofer

PHOENIX
dipole speaker

    Dipole models

    Active filters

    Microphone

     FAQ

Three-Box active
system (1978)

Reference
earphones

Surround
sound

Loudspeaker
& Room

 

 

Assemblies

LX521

ORION

PLUTO

Do-It-Yourself

 

 

Resources

Publications

Sound recordings

Links

Other designs

My current setup

About me

Site map

 

 

Conclusions

 

 

HOME

 

--------------------
ORION
PLUTO
LX521

Users Group

 

 

--------------------
Digital Photo
Processes

 

 

What's new

 

 


    | Introduction | Specifications | Construction | Electronics | Supplies | Photos | Pluto-2.1

 

Construction of the enclosure

The enclosure consists of a wooden base box and two pipe assemblies. The pipe material is standard plastic Schedule 40 plumbing PVC (white) or ABS (black). When sanded, ABS turns to a matte gray and PVC to a matte white surface color. 
- K is a 28.5" long and 4" inner diameter (4.5" OD) pipe. 
- L is a 33" long and 1.58" inner diameter (1.9" OD) pipe. 
- N is a 1.5" long coupler with 1.9" ID, 2.25" OD.
- O is a 90 degree angle with 1.9" ID.
-  M is a mating 1.9" OD pipe piece of about 3.5" length depending on N and O length. 
- P is a rubber coupler for 4" Clay to 4" Plastic with a steel clamp to tighten it onto K. It is 4" long and has 4.5" ID for the plastic pipe end and 5.12" (130 mm) ID with a 9 mm rim for supporting the midrange/woofer driver. It is Fernco's part number P1002-44. 
Fernco has subsidiaries in Canada, Europe and Australia.
- Q and R are standard caps to close the pipes. 
The pipes are tied together 24" up from their ends for rigidity of the assembly.

Woofer T is glued with GE Silicone II Household Glue to the coupler rim. Tweeter U is shimmed with thin cardboard and press fitted into coupler N. All pipes are loosely filled with Acousta-Stuf sound absorbing material.

The base box S has outside dimensions of 12 x 8 x 4 inch and houses the electronics which are mounted on a 11.5 x 6.25 plate of 1/4 inch plywood. The box must allow for ventilation of the heat generated by the three power amplifier IC packages and the toroidal power transformer.

 

The woofer/midrange driver is a Peerless HDS Nomex 832873 (= 830873). The previously used 850488 is no longer being manufactured by DST/Tymphany and inventory of this excellent driver is depleted. The 832873 is its drop-in replacement for PLUTO. 

An alternative woofer/midrange driver was developed by Seas for this application, L16RN-SL (H1480-08). It is the preferred driver when PLUTO is used without additional subwoofers.  It can be purchased from Madisound. A few circuit component changes are required for its use. They are listed on the PLUTO owner page. 

The tweeter driver is an AURA NSW2-326-8A. It may be difficult to obtain at times, but I do not have nor know of a substitute. It was actually this tweeter that inspired the PLUTO design.

The use of pipe K as enclosure for the woofer has advantages over a closed box. A pipe is inherently a very rigid structure and will not contribute secondary sound radiation from its surface. This is very difficult to avoid with a box construction where often wall vibration modes store energy and radiate more sound at certain frequencies than does the speaker cone. Pipes have a serious problem, though, in that they form acoustic resonators whenever their internal length is a multiple of a quarter wavelength. For PLUTO this is at multiples of 90 Hz, but can be well damped with stuffing as seen in a terminal impedance plot for the woofer.

It took some effort arrive at this result. The first prototype had a coloration of sound that could be detected with some broadband signals even though I thought the impedance curve looked acceptable. When I checked in the time domain the response to a 4-cycle Blackman windowed burst with the microphone very close to the dust cap of the woofer cone, I saw the picture at left. The delayed reflection off the rear end of the closed tube K is clearly visible as it is transmitted through the cone. Experiments with partially opening the rear of the pipe did not lead to improvements. 

A pipe that is closed at its far end has an extremely high acoustic terminating impedance, p/v, which presents a large mismatch to the pipe's own acoustic impedance. Openings at the end lower the terminating impedance, but also make it reactive due to local acoustic mass. The best result was obtained by leaving the pipe closed at its end and using just the right amount of stuffing material to absorb and not to reflect the rear wave coming off the cone. As seen in the right picture the reflection is now over 40 dB down. This represents acoustic waveguide propagation with over 40 dB return loss or less than 1% reflection. The long length of the pipe allowed for forming a very good acoustic resistor. The earlier sound coloration is no longer noticeable.

 


    | Introduction | Specifications | Construction | Electronics | Supplies | Photos | Pluto-2.1

 

 
What you hear is not the air pressure variation in itself 
but what has drawn your attention
in the two streams of superimposed air pressure variations at your eardrums

An acoustic event has dimensions of Time, Tone, Loudness and Space
Have they been recorded and rendered sensibly?

___________________________________________________________
Last revised: 06/28/2014   -  1999-2014 LINKWITZ LAB, All Rights Reserved