WG290Py
- Polyimide Driver + Horn
- 6.1″ x 6.1″ x 6.5″ Depth
- 109 dB – 180 Watts
This product is discontinued
and no longer available.
Features
Features

The compact and powerful WG290Py from PRV Audio combines a polyimide compression driver with a wide dispersion horn.
The specially designed polyimide diaphragm sounds very similar to the silk and textile dome tweeters used in high-end home audio speakers and studio monitors. PRV Audio combines this diaphragm with a high-energy motor for high-output over the usable driver bandwidth for effortless, dynamic output.
This combo offers an unsurpassed, natural upper-midrange and high-frequency response with authority. A 60° H x 60° V wide dispersion horn constructed from non-resonant recycled plastic, delivers space-filling sound at extremely high SPL levels. Acoustic loading is maintained down to 900 Hz.
Highlights
- Throat Diameter: 1″
- Type: Combo
- Nominal Impedance: 8Ω
- Rated AES Power Handling (RMS): 90 Watts
- Program Power: 180 Watts
WARNING: Cancer and Reproductive Harm – www.p65warnings.ca.govTechnical Details
GENERAL SPECIFICATIONS
| Exit Throat Diameter | 1” (25.4mm) |
| Nominal impedance | 8 Ohms |
| Rated AES Power Handling (RMS) | 90 Watts |
| Program Power | 180 Watts |
| Sensitivity 2.83V at 1m | 109 dB |
| Recommended Hi Pass Crossover** **For Full Power Handling |
1000 Hz** **12db Per Octave Crossover |
| Frequency Response at -10dB | 650 – 19,000 Hz |
| Voice Coil Diameter | 1.75″ (44.4 mm) |
| Voice Coil Wire | Copper |
| Voice Coil Former Material | Kapton |
| Diaphragm Material | Polyimide |
| Flux Density | 1.85 T |
| Magnet Material | Ferrite |


EXTRA INFO
| Overall Depth | 6.85” (174 mm) |
| Mounting Depth | 6.48” (164.5 mm) |
| Overall Width | 6.10” (154.7 mm) |
| Overall Height | 6.10” (154.7 mm) |
| Baffle Cutout Diameter | 5.11” (130 mm) |
| Net Weight | 2.86 lbs (1.3 kg) |
| Shipping Weight | 3.24 lbs (1.47 kg) |
| Carton Dimensions W x L x H | 7.08” x 6.69” x 7.08” (180 x 170 x 180 mm) |

Repair Parts
Replacement Diaphragm for WG290Py



