Modular active 3 way - work in progress

The sides were scalloped out, to reduce the baffle width. Its helps, but the wavefront starts to deform at 3Khz and there is some scattering by 4.5Khz. It think it could benefit from more rounding at the corners and a longer (Z>14cm) scallop. This was a simple cylindrical cut through the edges with some roundover. It's better than a flat baffle <2Khz but choppier above 2Khz.

.
 

Attachments

  • 3d_perspective.jpg
    3d_perspective.jpg
    68.7 KB · Views: 430
  • HpolarContour.jpg
    HpolarContour.jpg
    25.1 KB · Views: 428
  • Hpolar@3m.jpg
    Hpolar@3m.jpg
    38.8 KB · Views: 426
  • HField@750Hz.jpg
    HField@750Hz.jpg
    26.3 KB · Views: 429
  • HField@1K2Hz.jpg
    HField@1K2Hz.jpg
    27.3 KB · Views: 423
  • HField@3KHz.jpg
    HField@3KHz.jpg
    27.6 KB · Views: 49
  • HField@4K5Hz.jpg
    HField@4K5Hz.jpg
    27.5 KB · Views: 54
Last edited:
A longer scallop would provide a smoother transition but would also interfere with a desire to make the speaker modular so I can swap parts. The scallop is not required for the woofers or other potential midrange solutions (cones or horns). So its preferred to have a localized solution.

The midrange sims were used to see how much dome related variation was inherent in the cabinet and whether it could be further reduced.
 

Attachments

  • DSCN7821crop.jpg
    DSCN7821crop.jpg
    165.3 KB · Views: 110
  • DSCN7822crop.jpg
    DSCN7822crop.jpg
    243.6 KB · Views: 125
Last edited:
On to some more listening with the quad woofers setup and MF/HF horns replacing the domes.

It is much more effort to get everything aligned because the driver coil positions vary so much due to the horn length differences. The horns are moved to time align the drivers and eliminate the MF and HF nulls. Then a bunch of EQ was applied to flattened the FR@1m until I have something that measures like the dome solution. A single BP6 sub (80Hz) is used and there are some LF room issues (nulls) showing up.

I should add that my MF driver PRV290py-B does not go low enough to cross properly at 725Hz. The SH402 horn is suppose to load to 400Hz so I think it's driver limited. I can EQ the FR flat but the intended lower MF slope (LR4) is not correct. I added a midrange CSD and FR graph to show where it falls short. The HF horn has no problems.
 

Attachments

  • DSCN7822crop.jpg
    DSCN7822crop.jpg
    243.6 KB · Views: 133
  • Quads+SH402+DE07E - Time+Freq EQ FR.jpg
    Quads+SH402+DE07E - Time+Freq EQ FR.jpg
    78.8 KB · Views: 103
  • Quads+SH402+DE07E - Time+Freq EQ THD.jpg
    Quads+SH402+DE07E - Time+Freq EQ THD.jpg
    91.2 KB · Views: 75
  • LR4 BP + PRV290py + SH402  FR.jpg
    LR4 BP + PRV290py + SH402 FR.jpg
    80 KB · Views: 90
  • LR4 BP + PRV290py + SH402  CSD.jpg
    LR4 BP + PRV290py + SH402 CSD.jpg
    123.4 KB · Views: 86
pressure response vs power response

These trial systems were EQ'd to have approx the same axial response (ie. SPL@1m). The directivity is not the same so the power response of these speakers is also not the same. All the acoustic power emitted is in the room and should effect the sound.

So it should be possible to derive the power response using the pressure response and polar curves. Does anyone actually do that ??? is there a s/w tool ?
 
Hello Don,



You asked: So it should be possible to derive the power response using the pressure response and polar curves. Does anyone actually do that ??? is there a s/w tool ?


That is what Vituixcad was designed for. There is a separate window for DI and Power response. Additionally "heatmaps" can be displayed.
 
I think its the SPL integrated over the radiated surface area (so the directivity counts). I thought I read once that it could be estimated using only several measurements at different angles/distances. Still trying to find that. It would be even better if a tool did the calc for me.
 
I think you are looking for the ANSI / CTA 2034 standard aka "spinorama" this will show you how the different standard responses such as early reflections and power response are generated.

True power response is quite an effort to measure. Early reflections is the closest to how a speaker will measure in a room above transition.

Copy attached
 

Attachments

  • ANSI-CTA-2034-A_pdf.zip
    1.4 MB · Views: 108