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ORION support

Here you will find updates and new information for building your ORION speakers and for obtaining the best performance from them.

Note: All material is copyrighted and for the personal, non-commercial use by the person who bought it from LINKWITZ LAB. It may not be passed on in any form for use by others. | Terms & Conditions |

Please understand that I do not have the time to help you individually. Study my website and contact the OPLUG forum if you get stuck.

Access to the Resource pages of the ORION/PLUTO/LX User Group (OPLUG)
Now that you are a registered LXmini owner by having purchased the Construction Plans, you may have access to all the closed Resource pages. Forum registration is done by simply visiting this link and then responding to an automated email message. 

After you have registered, please forward proof of purchase to the OPLUG administrator: orionusers@gmail.com. The admin will then grant you unrestricted access to all site content.

 

 

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(67)  14 July 2013 - Support pages for the orion-4 ASP pcb

orion33_newpcb.htm       orion35_newpcb.htm

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(66)  22 March 2013 - Experimenter's Corner

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(65)  19 January 2013 - ASP impulse responses

Here are ARTA impulse response data (*.pir) from my ORION-3.3 ASP

TP2B - Woofer- Woofer cut - Mid - Tweeter

======================================
(64) 23 November 2012 - ASP output noise

Here are measured noise voltages for woofer, mid and tweeter outputs from my ORION-3.3 ASP. The voltages are displayed in dBV/sqrt(Hz), i.e. relative to 1 Vrms of noise in a 1 Hz bandwidth. Thus -140 dB/sqrt(Hz) corresponds to 100 nV per 1 Hz bandwidth, or to -97 dBV (14 uVrms) in a 20 kHz bandwidth. Normal hearing has the highest sensitivity around 3 kHz (Fletcher-Munson curves). The blue bottom curve is the noise floor of my E-MU Tracker-Pre sound card with shorted input. Visible are also 60 Hz power line and harmonics plus some spurious signals (probably my laptop) in the kHz range. It is important to chose a Kaiser window to separate the continuous signals from the random noise. I checked the accuracy of the measurement with calibrated noise and sine signals from the NTI Minirator MR1.

    Noise-orion33-woofer.png (32267 bytes)W   Noise-orion33-mid.png (33196 bytes)M   Noise-orion33-tweeter.png (32048 bytes)T           Noise-1mVsine.png (31881 bytes)  1 mVrms, 1 kHz sine

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(63)  4 December 2011 - Experimenter's Corner 

On this page I share with you some investigations that Don Barringer and myself are pursuing. You might want to experiment along those lines yourself and to give us feedback. In such case send me an email describing your observations.

======================================
(62)  20 October 2011 - ORION-3.5 conversion

Version 3.5 uses four of the SEAS L26RO4Y D1004-04 woofers in a W-frame configuration that fits exactly into the space of the current H-frame. 


Front

Rear
The photos show an example of a W-frame of equal width and construction as required for ORION-3.5

 

The difficulty with this design lies in aligning the multiple wood panels so that the box is square in the end.

I hold everything together with screws and pre-drill the holes. Adding glue makes for a slippery alignment unless you use fixtures. The two SEAS woofers are very massive and develop considerable forces, which must be absorbed by the cabinet. Using glue in addition to screws is desirable.

Left and right curved dress panels are screwed from the inside to the 1/4 inch thick hardboard side panels. All other panels are made of 3/4 inch multi-layer plywood.  

Cabinet drawing and cabinet parts list

Electrically v3.5 requires the addition of a 213Hz notch filter.

Otherwise the woofer channel is identical to v3.4 with 
R60 = 4.22k
R63 = 7.5k

Tweeter and midrange channels are identical to v3.3 and v3.4.

======================================
(61)  5 October 2011 - ORION-3.4 conversion

The SEAS L26RO4Y D1004-04 woofer has a larger magnet structure and greater excursion capability than the Peerless XLS 830452. To benefit from this requires an amplifier with higher power than the AT6012 such as the AT1806. Also, the bottom woofer's magnet would protrude past the grill cloth unless it is mounted with a wooden spacer Q of at least 5/8 inch (16 mm) thickness.  The outline of part Q is a 12 x 11.5 inch rectangle with a centric through-hole of 240mm diameter. The 11.5 inch width must have 2 x 3/4 inch cut-outs at the two bottom corners to clear parts J. 

For ORION-3.4 change the following resistor values on the old or new pcb:
U10B stage:  R60 = 4.22k & R63 = 7.5k
U11B stage:  R302 = 21.5k & R304 = 16.2k & R306 = 61.9k,  (C302 = 120nF, no change)

On the PHOENIX pcb change:
U9B stage:  R60 = 4.22k & R63 = 7.5k
U1A stage:  R2 = 82.5k & R3 = 28.7k,  (C2 = 120nF, no change)

======================================
(60)  20 August 2011 - Circuit diagram for Revision 3.3.1

Page 1 and Page 2  of the circuit diagram for update (59) when using the original pcb (Rev.120103 orion-2).
For circuit analysis and theoretical frequency response graphs use CircuitMaker or other SPICE program.

======================================
(59)  6/9/11 ORION Revision 3.3.1

There has been some further refinement of capacitor values for v3.3:

U7B stage:
C306 = 22nF (21.9nF optimally)

U1A stage   See (63)
C7 = 390nF  +/-40nF?? (390nF seems to be a reasonable value if you do not want to experiment)
The SHP affects the acoustic response in the discrete modal frequency range of the room. A universally correct value for C7 is not realistic, given the variations in rooms and loudspeaker placements. But there seems to exist an optimum value for each setup.

U3A stage
C208 = 120nF (39nF in parallel with existing  82nF)

Unchanged from (57) below:
R22 = 1.96k
R24 = 4.22k
C28 = 56nF (54.8nF optimally)
R400 and C400 removed from R4

Agilent Technologies makes a U1701B Handheld Capacitance Meter ($158) that was used to measure the optimum values, 
otherwise capacitors have 2% tolerance.

The material list has been updated by BrianL.:  orion331_BOM_2011-06-09.xls 

======================================
(58)   5/6/11 ORION Revision 3.3

After hearing ORION-4 at AXPONA in Atlanta for the first time and noting the differences to his ORION-3.2.1 Don Barringer went home, lowered the midrange crossover frequency to 92Hz and reduced the output at the top end of the midrange driver slightly. The sound now matches ORION-4 closely, except for some of the articulation and dynamism that the new SEAS woofers deliver. When these new drivers become available, I will try them in the H-frame and publish here the necessary ASP and cabinet changes.

U2A, U2B, U9A, U11A stages:
R57, R58, R208, R211, R221, R222  = 26.1k
R209, R212 = open
R210, R213 = 51.1k

U7B stage:
C306 = 22nF (22.0nF to 22.2nF optimally)

U1A stage
C7 = 377nF (330nF in parallel with 47nF)   See (63)

ORION-3.3 circuit diagrams for ASP pcb: Page 1, Page 2, component layout and ASP frequency response
If (57) has been implemented, then add 3.3dB to woofer, mid and tweeter levels.

The material list has been updated with the help of BrianL, DpB and others competent to give inputs. Thanks for your help. orion33_BOM_2011-06-03.xls 

Don and I highly recommend that you make these changes to your ORION-3.2.1 ASP, but neither of us nor Wood Artistry can provide an upgrade service at this time.

NOTE: When used with THOR the increased phase-shift from the 92Hz crossover will influence the integration of the woofer with ORION-3.3. See https://www.linkwitzlab.com/frontiers_5.htm .

For the Phoenix-MT1 pcb version of the ASP:

MT1- U4A, U2A, U2B stages:
R21, R22, R8, R11 = 26.1k
R9, R12 = open
R10, R13 = 51.1k

Ph - U9A, U10A stages:
R57, R58 = 26.1k
C73 = 22nF (22.0nF to 22.2nF optimally)

Ph - U1A stage
C7 = 377nF (330nF in parallel with 47nF)  See (63)

ORION-3.3 circuit diagrams for Phoenix-MT1 pcb: Page 1, Page 2 (both corrected 12/30/11) and ASP frequency response
If (57) has been implemented, then add 3.3dB to woofer, mid and tweeter levels in the frequency response graph.

======================================
(57)   4/10/11 Preamp with high output impedance

If the output impedance of your preamp is greater than 200 ohm, then do not install the R400-C400 1.8kHz shelving lowpass filter.
To obtain the desired frequency response install instead:

R22 = 1.96k
R24 = 4.22k
C28 = 56nF (54.8nF optimally)

The gain in each ASP channel will increase by 3.3 dB as a consequence, but that should not be of concern.
This change can also be applied to the Phoenix/MT1 pcb based ORION provided that the -3dB/dec slope filter has not been installed or is removed. Then add a jumper wire from the C28-C27 junction to the R22-R24 junction

======================================
(56)  10/10/10 ORION Revision 3.2.1

Change C7 from 330nF to 390nF (or 330nF in parallel with 56nF)
This provides an increase in upper and lower bass output for improved overall balance and a reduction in dryness.

Customers who paid for an upgrade to Rev. 3.2 can obtain this latest revision from Wood Artistry for $20 plus S&H. The change for item (55) below will be included, but could be less desirable for warped vinyl playback. Please indicate your preference.

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(55)  10/10/10  Change of 50Hz HPF to 30Hz

Reducing the S1 switched cut-off frequency of the 50Hz highpass filter to 30Hz extends the useful low frequency response, while still being effective in reducing subsonic cone displacements of the woofer drivers. It allows for higher volume levels with little loss at the low end. It is a useful mode for some recordings that cannot be played adequately loud otherwise.

If C100 = 150 nF, change R100 from 21.5k to 34.8k
If C100 = 120 nF, change R100 from 26.1k to 42.2k

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(54)  7/26/10  ORION Revision 3.2

The required components are listed on the Revision 3 Materials and System Tune-up page. The circuit conversion takes 3 to 4 hours of soldering and testing. The system tune-up is likely to take considerably longer, but is necessary to hear all the benefits of this revision.

I am aware of and frustrated by the shortage of 2% tolerance and low loss capacitors. Don Barringer has been trying to find new suppliers for the parts he needs. We know that useable parts are still being being manufactured in the US and Taiwan and probably in China in large quantities, but they are not handled by the known distributors for small quantities. The tolerance is important, the loss factor and film material are much less so, because the capacitors are often in series with large resistors. Other than the parts availability issue it should not be too difficult to modify the ASP since you already have the experience from building it yourself.

If you did not build the xo/eq yourself and bought it from us, then contact Don Naples from Wood Artistry for a Return Material Authorization (RMA). Don has all the test equipment and experience. He worked in the electronics industry most of his life. Wood working used to be his hobby. But do not just send the xo/eq to him. He needs to schedule the upgrade according to his time and material availability and you may not want to be out of a working Orion for a long time. Right now he is gone fishing until August 1. 

Your cost for the upgrade service is $290 plus shipping and handling. 

Don can also work on DIY assembled crossovers, but this may result in additional charges. Ask for a quote

If necessary, I will try to recruit others to help out. For pay of course. If you think that you are skilled and have the test equipment to perform a Revision 3 upgrade that would meet my quality standards, then send me an email

======================================
(53)  2/25/10  ORION+

There has been some concern that the ORION documentation has not been updated to the ORION+ to show the rear tweeter mounting and midrange driver mounting.

The rear tweeter mounting is described on the ORION++ page. I would change the panel thickness from 3/8" to 3/4" to increase stiffness, thus to 11-3/8" x 6" x 3/4" and the two side supports to 6" x 1" x 3/4". Round or chamfer the corners as in the Wood Artistry example.

The midrange driver mounting is described on the Revision 0.1 page. The key difference to the obsolete mounting bracket, where the magnet was glued to a wooden puck, is the use of a long screw through the center of the magnet, a replacement of the screw that holds the copper bullet of the driver, to attach the driver magnet to its wooden support. The Wood Artistry kit uses this technique. You could use the same approach in your own design of the mounting bracket.

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(52)  9/2/09  ORION/PLUTO Users Group log-in

Now that you are an ORION owner/builder you can request access to the locked areas of the forum.

Sign in with your email and a password at https://oplug-support.org/index.php . You will be refused access but you can send an email to the Board Administrator (orionusers@gmail.com) from there and request to be admitted as an owner.

======================================
(51)  11/25/08  Obsolete capacitors

For polypropylene capacitor replacement use the Panasonic ECHS-Series of PPS film capacitors with 2% tolerance and 50 (or 100) WV DC rating. (e.g. 33nF = PS1H333G-ND)

It appears that the ECSH series will be continued for some time. The increased dissipation factor of 0.3% for PPS compared to 0.1% for PP should have no sonic effect.

For polyester film capacitor replacement use the Panasonic E-Series. (e.g. 10uF = E1106-ND)

For updates and help also check in with the ORION/PLUTO Users Group

======================================
(50)  11/3/08  ORION+ rear tweeter level adjustment

You may have missed the update to the ORION++ page a while ago. It was heavily based on inputs from John Stone. If you have concerns over the ORION's top end, then here is the way to experiment. Unfortunately the proper level setting is very critical and can be room dependent. 

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(49)  8/23/08  ORION Material List

Updated material list to account for obsolete Panasonic capacitors, DIN connector and rear tweeters.

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(48)  7/24/07 ORION Material List

The new DigiKey part number for the 1kohm trimmer potentiometer is  3362P-1-102LF-ND

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(47)  5/22/07 ORION+

Here is the concept that should guide the experimental optimization of your ORION+/Room/Listener system setup:

An electro-acoustic transducer needs to have a uniform (4p) power response and be flat on-axis under 4p/2p space conditions. Then it illuminates a room uniformly. This allows perceptual separation of the room sound from the direct sound. Room effects are minimized, if the room reflections arriving at the listener are delayed sufficiently, and if they replicate the direct sound sufficiently. 

======================================
(46)  5/13/07 ORION+ 

If you have any complaints about the high frequency response of the ORION+, then please consider the following:

1 - The ORION+ will reproduce what is on the recording and what has been added to it in the signal path before the speaker driver terminals. But the recording dominates.
2 - You must optimize the ASP tweeter level setting by listening even if the ASP measures perfectly. Midrange and tweeter sensitivity has production variations.
3 - Since you have little information about how a recording was made and processed you should listen to multiple recordings. Avoid studio recordings and those done with large numbers of microphones. That probably leaves you with some classical recordings and live (un-amplified) jazz. Forget about pop, rock, electronic, etc, recordings. Choral works and good voice recordings in natural settings can be revealing.
4 - Most important of all, observe live sounds and do not use your memory of a loudspeaker as your target.

Have fun discovering what's in the ORION+.

======================================
(45)  4/21/07  Rear tweeter and ASP (ORION+)

Here are, after various iterations, the circuit and adjustment changes that resulted from the addition of the rear tweeter (Seas T25CF002, Millennium). 

a) The rear tweeter is wired in parallel to the front tweeter and with opposite polarity. Both tweeters are driven at the same level. No series resistor is used. 
b) Dipole EQ    R55 = 3.24k     (unchanged: R54 = 38.3k, C64 = 120nF)    
c) Notch Filter    R51 + R307 = 4.75k     (unchanged: C61 + C62 = 42.3nF)    
d) The ASP tweeter level is set around 2 ticks down.
e) Check if the ASP woofer level is set optimally. It might require a 1 tick increase.

(45b)  5/5/07  
I find it a bit disturbing how critical the ASP level settings are. Half a tick (0.25 dB) for the tweeter makes a noticeable difference in overall sound balance. So experiment and judge by long-term listening to different source materials. You will recognize by its naturalness when you have it optimized.

======================================
(44)  3/3/07  New DigiKey part numbers 

220pf ceramic caps are 1404PH-ND
THOR 10k potentiometers are 3362P-103LF-ND 

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(43)  1/23/07

Very important !!!

If there is a crimp connector on the wire attached to the tweeter (rather than a solder connection), use extreme care when pulling the wire connector off of the tweeter terminal or you can damage the tweeter by pulling out the tweeter terminal. You can use a screwdriver to hold the "T" part of the terminal in place while removing the wire connector from the tweeter.

If you pull the terminal out of the plastic you rip the tweeter's lead-in wires! The repair requires opening the tweeter and becomes a delicate operation.

======================================
(42)  12/23/06, 7/7/08

In case you ever need to replace the voice coil assembly of your tweeter, here is the procedure for re-assembly:

Before you fully tighten the front plate, apply a 2 volt sine signal at 500Hz.  Push the front-plate to try to stop any distortion and tighten the screw closest to this point first.  (This low frequency allows large excursions without much sound to better identify mechanical noises.)
If this doesn't work, assemble the dome and apply the above signal so that you hear any distortion. Then use your fingertip and gently push down on the surround of the dome and move your finger around the circumference. This may put things in alignment. 
A tip regarding ferro-fluid: It is important to remove the voice-coil assembly slowly from the magnet system. Then the magnetic force will pull the ferro-fluid off the voice-coil and back into the gap. If it's the same voice-coil assembly you first take out and then put in, it's no problem. No fluid should be lost unless you wipe it off the voice-coil.

Bjorn Magne Idland
Laboratory Technician
SEAS, Norway

If you do not have a 500 Hz sine wave, then download 500Hz-sine.zip , unzip it and burn the file to CD. It will give you a 5 minute track of 500 Hz in normal stereo format. You can also download and install on your computer a virtual Minirator MR1 signal generator.

Note the O ring on the outside of the plastic assembly. This must be transferred from the defective vc to the new one. It provides an air seal.
As for the orientation, the voice coil to front plate orientation is fixed by the terminal mountings having slightly different cutouts. This means it can only go in one way and the positive marking on the plate will always correspond to the correct terminal.
The orientation of the replacement voice coil on the magnet system can be one of 2 ways-either the original, or 180 degrees rotated. It doesn't matter, as long as the terminals aren't rotated 90 degrees from the original orientation.
Finally, you should tighten the screws using the procedure outlined on the support page. Because of the gaskets, the torque has to be evenly applied to prevent rub and buzz.
This is done very precisely in manufacturing, but of course that precision is not available when replacing the voice coil assembly yourself. (John Stone - Seas)

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(41)  11/14/06

When the Test Table on page 28 of the 1/19/06 documentation was updated, I missed to change the value for Track 3, Mid out, from 0.68 V to 0.77 V.

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(40)  11/11/06 

A pdf copy of the full size Side Panel drawing was provided by Eric Snyder to make the construction of the template easier. 

======================================
(39)  10/2/06


Drawings by Sigurjon Hauksson

ORION+  2/17/07
The drawing shows the direction in which the driver cones must move when a positive dc voltage is applied to the positive speaker cable plug for each driver. All power amplifiers must be identical or have the same polarity and voltage gain. 

In the case where the ORION crossover/equalizer is built with two PHOENIX and one MT1 circuit board, the two woofer drivers must be wired to move in opposite direction from what is shown here, because the woofer output signal from this older crossover/equalizer has inverted polarity. This polarity inversion was later removed with the newer ORION ASP printed circuit board, but otherwise there is no functional change. 

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(38)  6/18/06

A substitute for the OPA2134 operational amplifier is the OPA2604. You could also use the TL072 until either one of them is available. I would be curious to know if you hear a difference.

====================================== 
(37)  5/4/06

ORION Revision 0.1v4, magnet mounting

From the inception of the ORION, several subtle equalization changes have been made to address the complicated interaction between the front and rear radiation from the midrange driver in the frequency region where symmetry is lost due to the concave driver cone on the front side of the baffle and the basket/spider/magnet structure on the back side of the baffle. The 400 NF notch filter and the 30-400 SLP dipole correction are instrumental for the on-axis frequency response. Further investigation since (36) has led to a change of the earlier (R51 + R307) value. It should be noted, though, that all these changes are of a magnitude where it becomes difficult to guarantee that they are optimum in an absolute sense. The components in the crossover/equalizer have finite tolerances and especially the midrange driver has variation in sensitivity, and to a lesser degree in frequency response shape, all of which can easily be of the size of the tuning adjustments being made here. Thus these updates should not be viewed as absolute and necessary for continued satisfaction. They are posted to signify a change in current production, giving current owners the option to either modify their systems as well or simply continue their present enjoyment without them. In any case, before modifying your electronics you should be quite certain that the woofer and tweeter level settings are optimum for your situation. They have much larger influence on the overall sound than these revisions. A 0.5 dB change in either level setting is quite significant to long-term listening enjoyment, even if the change is not immediately recognizable. Driver sensitivity can easily vary by 0.5 dB between different production units, but it can also be easily compensated in an active system like the ORION. 

For magnet or rim mount of the midrange driver: 
Dipole eq. (30-400 SLP): R54 = 38.3k and R55 = 3.16k
Notch filter (400 NF) capacitors: 
C61 + C62 = 42.3 nF measured (e.g. C61 = 39 nF and C62 = 3.3 nF) 

Notch filter (400 NF) resistors for magnet mount:
R51 + R307 = 4.53k (e.g. 4.42k + 100 ohms or 4.22k + 301 ohms)
Phoenix boards:  R51 = 4.53k

Notch filter (400 NF) resistors for rim mount:
R51 + R307 = 4.42k
(e.g. R51 = 4.22k and R307 = 196 ohm)
Phoenix boards:  R51 = 4.42k

======================================
(36)  4/12/06

ORION Revision 0.1v3, magnet mounting

After extensive listening and experimentation Don Barringer recommends the following: 

Change R307 from 196 ohm to 422 ohm to obtain R51+ R307 = 4.64k

Confirm that:
R51 = 4.22k 
C61 + C62 = 42.3 nF measured (e.g. C61 = 39 nF and C62 = 3.3 nF)
R55 = 3.16k
R54 = 38.3k

The assembled crossover/equalizer will be shipped with the changed R51+ R307 component value from now on.

For the rim mounted midrange there is no change from:
R51 + R307 = 4.42k, (e.g. R51 = 4.22k and R307 = 196 ohm)
C61 + C62 = 42.3 nF measured (e.g. C61 = 39 nF and C62 = 3.3 nF)
R55 = 3.16k
R54 = 38.3k

=======================================
(35)  2/25/06

The test table on page 28 of the ORION Construction Kit Documentation has been updated to capture the frequency response changes that were caused by Revision 0.1 v2. The table goes with the material list component values under (33) and represents current shipment practice for the assembled xo/eq regardless of whether the Conversion Kit has been installed or not.

Here is the current Test Table: 7-circuit test.xls

The resolution of the frequency response graph on page 27 is not sufficient to show the changes.

======================================
(34)  1/1/06

The 8-pin IC socket Assmann A08-LC-TTA08-LC-TT or  Digi-Key part AE8908-ND is no longer available.
Use instead Assmann A08-LC-TT-R, Digi-Key part AE9986-ND

======================================
(33)  1/19/06

The material list on page 21 is missing in some printings of the ORION Construction Kit Documentation

Here is the current list: 5-Orion-material.xls

Install the Excel 97/2000 Viewer on your computer, if you do not have access to the Microsoft Excel spreadsheet program. 

======================================
(32)  11/11/05

New DigiKey part numbers

100 pF is now P4570-ND
220 pF is now P4574-ND

======================================
(31)  9/9/05

Assembly instructions for the Wood Artistry flat-pack and for mounting the midrange driver according to Revision 0.1 when using the Wood Artistry Conversion Kit 1A.

======================================
(30)  8/22/05

On page 10 of the 6/16/05 documentation in the 4th paragraph: 
Change the writing "6x3/4" to "6x5/8". 
The McFeely's part numbers are correct.

======================================
(29)  7/7/05

You can download the ORION label file and print it out on premium photo paper. You might like to glue a 2" wide label to the front panel of your crossover/equalizer and a 4" wide label on top of the speaker's woofer baffle to help me promote the speakers.

======================================
(28)  5/1/04

Final cabinet assembly (page 4)

3M, Scotch Brand adhesive transfer tape 468MP is available on a 1" wide x 60 yard roll

======================================
(27)  3/30/05

No components are loaded on the ORION printed circuit board in the following locations:

R24, R34, R50, R68, R69, R301
C28, C70, C73, C301, C303, C304

These are place holders for different circuit applications.

======================================
(26)  3/4/05

ORION Revision 0.1v2, magnet mounting

Some further small changes were made to the midrange driver equalization which supercede (20) below. They add a little more warmth in the region below 400 Hz. 

A - On the ORION circuit board in the 400 NF section check that R51 + R307 = 4.42k, i.e. R51 = 4.22k, R307 = 196 ohm, or R51 = 4.42k, R307 = 0 ohm jumper. Check that C61 = 39nF. Change C62 from 4.7nF to 3.3nF. 
In the 30-400 SLP section change R55 from 3.48k to 3.16k and change R54 from 42.2k to 38.3k.

B - If the PHOENIX circuit board is used, then change R51 to 4.42k, change C61 to 39nF and add/change C62 = 3.3nF in the 400 NF section. In the 30-400 SLP section change R55 from 3.48k to 3.16k and change R54 from 42.2k to 38.3k.

These changes are not necessarily related to the magnet mounting and might be tried without it.

=======================================
(25) 11/19/04

Crossover/Equalizer power consumption

Each operational amplifier could draw 5 mA max of quiescent current. Allocate 10 mA per OPA2134 package plus 50% margin for a total of 15 mA/package. Thus, the power supply for 22 ICs should be capable of 330 mA. Average power consumption is about 5 W when using +/-12V. Do not exceed +/-18V.

======================================
(24) 11/17/04

Side panel material

The side panels do not need to be constructed out of multi-layer plywood. A variety of materials can be used, but they should not ring for lack of internal damping when knocked on. The panel thickness should be 3/4 inch to 1 inch maximum to maintain the desired acoustic path length from the rear of the midrange driver to the front, and to maintain the distance from the tweeter to the cabinet edge. See also (8) below.

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(23) 11/3/04

The McFeely screws are now available over the web: 

https://www.mcfeelys.com/

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(22)  8/19/04

Digi-Key Finland (https://fi.digikey.com/) might be a good source for electronic parts in Finland. They use the same part numbers as in the ORION material list. 
Also check out Digi-Key International (https://dkc1.digikey.com/us/mkt/International.html)

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(21)  8/18/04

Revision 1/26/04 of the Construction Kit Documentation.
Page 16, Circuit diagram. Change the value for C214 from 33nF to 47nF. The material list and loading table on page 19 are correct.

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(20)  8/18/04

ORION Revision 0.1, magnet mounting, requires a small change to the 400 Hz notch filter to bring up the response by about 0.5 dB.
A - On the ORION circuit board change R307 from 196 ohm to 422 ohm. Check that R51 = 4.22k, C61 = 39nF, C62 = 4.7nF.
B - If the PHOENIX circuit board is used, then change R51 from 4.42k to 4.64k. Change C61 to 39nF and add C62 = 4.7nF.

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(19)  7/13/04

For ORION cabinet work in the US contact Wood Artistry

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(18)  7/13/04

For ORION cabinet work in Australia contact Steven Rosenberg

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(17)  7/13/04, updated 3/20/06

For ORION cabinet work in the UK there is no longer a contact.

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(16)  5/5/04

Side panel drawing templates have been provided by Alister Sibbald:

US Letter format
US Tabloid format
A4 format
A3 format

The PDF files print out on multiple pieces of paper, making it necessary to match each piece with the next,  which is the purpose of the "crosshair" markings in each corner of each sheet. It makes things much easier if they are printed out on the most transparent paper available. If Transparency sheet is available, that is ideal, as it makes matching up the crosshairs extremely simple. Once you have taped up all the pages with Scotch tape, the resulting full size pattern can be glued to your template and used to cut it out. 
Each sheet is labeled with a legend such as "R1C1" to RnCn" standing for "Row 1 Column 1", which is the lower Left hand sheet, with R5C3 being the upper right hand sheet in the case of a drawing which extends over 5 rows and 3 columns, for
example.

See also the side panel drawing (9) below.

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(15)  1/30/04

Revision 1/26/04 documentation for the new ORION-ASP pcb.

On page 10, 2nd paragraph, it should read correctly: 
"... the two woofer cones move forward, when a positive voltage ..."

On page 4, Final cabinet assembly, add the underlined:
"Glue the finished dress panel to the painted midrange baffle using 3M, Scotch Brand, adhesive transfer tape 468MP. A 60 yard roll of 1/2 inch wide tape costs $14. https://www.rshughes.com/home.html.  Cover the whole dress panel with strips of tape.

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(14)

Adjusting the gain of the 3 crossover channels

The tweeter and woofer channels have trim potentiometers (R32, R61) to adjust the gain by +/-2.5 dB. This is a large range in order accommodate normal manufacturing variations in driver sensitivity, in the order of 0.5 dB, and differences in room acoustics and listener preferences. The normal position of the potentiometer is at the center of the tick mark range. The gain changes 0.5 dB between adjacent tick marks.

The XO/EQ was designed for power amplifier voltage gains between 24 dB and 28 dB. Amplifiers with higher gain degrade noise and hum rejection. All three (four, if woofers are driven individually) amplifiers should be identical. If power amplifiers of different voltage gain are used, then the potentiometers may have insufficient range and attenuators must be added to the output of the XO/EQ. The lowest gain amplifier determines by how much the input signal to the other amplifiers has to be attenuated. The 196 ohm output resistors (R43, 56, 64) must be replaced as necessary by a resistor R1. A resistor R2 must be soldered between the RCA output connector and nearby circuit ground. 

Determine the values of R1 and R2 from attnrout.gif by setting Rout = 2k ohm.  For example, a 5 dB attenuator (a=0.56) would have R1 = 3.56k and R2 = 4.56k. If the input impedance of the higher gain power amplifier is 10k, then the actual attenuation will be 20 log( (4.56//10)/(3.56 + 4.56//10) ) = -6.6 dB, which is higher than targeted. Thus R1 needs to be reduced and a modified R2' = 4.56//10 = 3.13k used in the formula for  R1 = R2'(1-a)/a = 2.44k. Choose the next closest standard value resistors. 

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(13) 

Reducing "Hum"

With many components connected to the power line there is the potential of "ground loops" which induce hum into the system. Ground loops are closed circuits which provide paths for low level AC ground currents to flow between different ground connections, if these connections are at different ground potentials, or if magnetic stray fields from power transformers induce currents into the loops. If the RCA cables which interconnect the different pieces of equipment are part of the loops, then the ground currents will also flow in the cable shields. Cable shields and associated RCA connector junctions have a finite ohmic resistance so that there is a voltage drop induced across that resistance by the ground current. A "hum" voltage is thereby added to the normal signal voltage. 
A quiet system has 1 mV or less hum and noise voltage, mostly 60 Hz and 120 Hz, at the power amplifier output binding posts. It takes a sensitive AC Voltmeter to measure this. Alternatively, listen with one ear close to each midrange driver to compare the amount of hum for different configurations.

  1. Make sure that all components are plugged into the same AC power outlet by using a power strip.
  2. The power amplifier has a three-wire AC cord with a safety grounding type plug. If any other component in the system uses such a 3-prong plug it may cause a ground loop. Turn off the power amplifier. Add a 3-prong to 2-prong adapter to each of those plugs, one at a time, except for the power amplifier. Each time turn on the power amplifier to check if the hum has disappeared. For safety reasons never isolate the 3rd pin of the power amplifier plug!
  3. If you have a tuner in the system with Cable TV connection, then disconnect the cable. If the hum disappears, you must insert a Ground Loop Isolator before reconnecting the Cable.
  4. Make sure the Crossover/Equalizer is not located close to a component with strong stray magnetic fields from a transformer.
  5. Make sure that all interconnect cables have clean contacts and are plugged in tightly.
  6. Change the three crossover outputs to reduce the crossover gain by 10 dB and thus increase the signal to hum ratio by 10 dB. Consequently the preamp volume control needs to be turned up 10 dB higher.
    Replace the 196 ohm resistors R43, R56 and R64 with 3.83k resistors. Add three 1.96k resistors and solder them from each RCA output connector center pin to a nearby ground. This adds 10 dB output attenuators to the tweeter, mid and woofer channels.
  7. If all fails, use a Jensen-Transformer ISO-MAX Ground Isolation Interface. Their model CI-2RR costs $180 and is externally connected to the inputs of the Crossover/Equalizer. There is no need for balanced inputs since the Jensen unit has isolation transformers build in. They block ground loop currents from flowing and causing hum.

The AT6012, for example, is a very quiet power amplifier. I measure less than -80 dBV (<100 uVrms) hum and noise across its output binding posts with the RCA inputs short-circuited. The measurement is performed with a NTI Minilyzer ML1, which has balanced inputs. When there has been a hum problem in any of my systems, it was never due to one of the different ATI power amplifiers that I have used over the years.

See also ORION FAQ10.

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(12)

Spaekon connectors

Note, the following alternative is not recommended when building the speakers yourself, because of potentially lower reliability of connections due to increased difficulty in assembly. These parts are used on the custom assembled ORION System to simplify the speaker setup for the user. There is no sonic benefit over the solution in the Construction Plans+. 

Instead of soldering the speaker cable to a solder terminal strip at the speaker end we install a Neutrik 8-pole Speakon connection. The part numbers in the Mouser catalog are:

568-NL8MPR-BAG male, chassis, Faston tabs,  $7.28
568-NL8FC female, cable, screw terminals,  $10.44

For a Belden 8-conductor cable 1811A we make the following connections to minimize crosstalk:

Tweeter: blk-wht
Midrange: brn-blu
Woofer top: grn-red
Woofer bottom: yel-org

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(11)  8/7/03

Revision 4/18/2003 documentation

Page 27, CD track 2, Tweeter out =  0.42 +/- 0.02,  not 0.40 +/- 0.02

C62 = open, not 12 nF

C8 = 100 nF on MT1 loading chart, not 82 nF 

Material list and loading chart

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(10)

If Digi-Key is out of stock on a certain part, ask for an alternate part with the same value and tolerance. Voltage and Wattage ratings are not critical. I like to order over the phone to make immediate adjustments (1-800-344-4539). For example, the Yageo 3.48K, 1% resistor (3.48kXBK)  can be replaced by a BC Components resistor (BC3.48KYCT).  Another good source for parts is Mouser.

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(9)

Side panel drawing with curve radii.
If the actual dimensions of the side panel are within +/-1/4 inch of the drawing on page 7, then the acoustic properties remain unchanged.

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(8)

Any material can be used for the side panels, plywood, MDF, solid wood, Plexiglass, Corean etc. as long as it is sturdy. The edges can be rounded or beveled. None of this has an effect on the sound as long as the outline of the side panel remains unchanged and it is firmly attached to the internal frame. 

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(7)

Revision 10/16/02 documentation updates:

Page 4
When aligning the curved side panel with the frame, then the front edge of the panel at the top should be flush with the surface of the dress panel. This forms a 1/4" deep grove to the side of the dress panel for cosmetic and acoustic reasons. The side panel sticks out 1/2" from the frame at the bottom.

Page 9
After the drivers have been inserted and screwed down wait for a day and then check tightness of the mounting screws. The weather strip foam tape will  have taken a set. This is desirable. You should not use a hard rubber gasket material that remains springy. It might cause buzzing distortion when the driver frame hits the mounting screws. 
The material should be pliable. For example, a Frost King vinyl foam weather seal V212G (charcoal) or V443 (gray) works well. It is 3/16" thick x 3/8" wide. 

Page 15
Add C11 (220 pF) in parallel to R19 at U3B of the 120 PH stage.

Page 17
Increase used quantity for the 220 pF ceramic capacitor from 8 to 12.

Page 20
Add to the loading chart for the MT1 pcb four 220 pF ceramic capacitors in locations C9, 11.

Page 21
One of the LED can be mounted to the front panel as indicator light. If it is too bright, then increase R27 to 10k.

Page 26
A - Spot check of xo/eq transfer function magnitude and phase.
The 50 HP switch must be closed to defeat the low frequency cut. 
The woofer, mid and tweeter output voltages are measured from the hot center pin to ground. The difference voltages W - M and M - T are measured with the leads of the DVM clipped to the hot center pins of woofer and mid and then mid and tweeter.

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(6)

Back-ordered Substitute Digi-Key
3300uF, 25V 2700uF, 25V P10286-ND
68nF polypropylene 68nF polyprop. film P3486-ND

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(5)

Material list and loading chart

Install the Excel 97/2000 Viewer on your computer, if you do not have access to the Microsoft Excel spreadsheet program. 

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(4)

Revision 10/14/02 documentation 

- Correct page 21

- Page 18 
    21.5k resistor, 4 used, not 14 (R100 - Phoenix and R1 - MT1)

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(3)

Before Revision 10/14/02 documentations

- Page 5
    D = Hardwood
    K = Hardboard or Masonite for the template

- Page 14
    Correct C65 = 47 nF on circuit schematic 

- Page 11, 17, 18, 19, 20
The online crossover/eq material list spreadsheet has several updates and corrections for components and their placement. Print out and use the spreadsheets to order and load parts. Click on the tabs at the bottom of the spreadsheet to see the three different lists.

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(2)

The Orion design was frozen August 1, 2002.
The changes above are only corrections to the published material. Unfortunately errors crept in when generating and duplicating the documentation.

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(1)

Assembly of the ORION

Front and rear view of the internal frame before it is painted flat black. The finished dress panel is glued to the top section of the frame later on.

 

The side panels have been attached to the internal frame.
The dress panel is still missing.
The frame is ready for mounting the drivers, but care must be taken that the top two drivers are centered in the dress panel holes. 

 

Rear of top panel.

 

Wiring of the 4 speaker cables to terminal strips inside the cabinet.

 

Crossover/Equalizer prototype.

 

 


| ChallengeConstruction Kit |

 

 

What you hear is not the air pressure variation in itself 
but what has drawn your attention
in the 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: 02/15/2023   -  © 1999-2019 LINKWITZ LAB, All Rights Reserved