£ Trade
• 1,000W @ 2/4 Ohms or 70V per channel
• 500W @ 8 Ohms per channel
The CA-1.02 Class D Power Amplifier is capable of driving up to 1,000W at 2 or 4 Ohms or 70V per channel, and 500W at 8 Ohms per channel. In Bridge Mode, it can deliver 2,000W at 8 Ohms or 100V, providing powerful performance for demanding installations.
Its robust design makes it ideal for high-fidelity directional sound applications, ensuring focused and clear audio in professional environments.
| No. of Channels | 8 |
|---|---|
| Output Stage Type | Class D |
| Units Rack Space | 2U |
Class-D switching amplifier technology.
Stable at 2 Ohms, separate switch-mode power supplies auto detect 120VAC or 240VAC operation and increases reliability and performance.
NX chassis are lightweight and feature highly-conductive Galvalume® steel construction that provides the ultimate in low-noise shielding and EMI suppression.
Multi-Mode operation offers flexibility.
NX maximizes rack density by mixing operation modes to dial into whatever the system requirements demand.
Set the DIP-switch configuration on the rear panel to select Low Impedance (2, 4, and 8 Ohm), or Constant Voltage (70V or 100V) and you’re set to go.
Energy-efficiency out of the box.
We’re doing our part to conserve energy. NX features power-saving Ashly EMS™(Energy Management System) and is offered exclusively across the entire NX line.
Ashly EMS is a defeatable <1W sleep-mode that complies with the most aggressive Energy Star®benchmark.
Network audio keeps you connected.
Optional Dante® or CobraNet® integrate media and control for your entire AV system over a single IP network.
Each card is factory-installed with your order and easy to configure right out of the box. (nXe and nXp models only)
FREE remote control for Apple iPad,® called Ashly Remote.
Design and deploy custom remote control interfaces to control the amplifier over WiFi. Add controls specific to your system by designing menu systems, faders, assign text labels, toggles, fixed presets, and much more.
Hardwired Ashly Remotes are available including passive (all models), serial data, and Ethernet remotes. (nXe & nXp models).
Audio professionals find our software very intuitive—and you will too.
No need to attend a one-week training class to learn our software―common sense layout of controls and features make it easy to navigate.
Features include: Auto mixer, feedback suppressor, ambient noise compensation, dynamics processing with auto-ducking, and much more.
We’re committed to high standards in sound clarity.
Backed by our team of engineers and a 5-year worry-free warranty, our goal is to always give you years of uninterrupted service.
nX is hand-built in Webster NY.
We are passionately focused on providing audio clarity for you and your clients. With over 40 years in the audio business, you’ll find our service after the sale is unmatched by any in our industry.
| 24 Total Inputs x 14 Mix Buses |
| 16 Discrete Ashly Class-A Mic/Line Combo Inputs (-126dBu EIN) |
| Dynamic Range >110dB |
| 32-bit ADC, DSP and DAC |
| 24 x 8 Aux Channels or 24 x 4 Aux / 4 Sub |
| Stereo Solo any Channels or Mix Buses |
| 8 Separate Aux Outputs |
| 8 Separate Channel Inserts |
| 33 Channels of DSP Processing: Expander/Gate, Comp/Limiter, PEQ |
| 2 Stereo FX Processors: 12 Digital FX: Reverb, Delay, Chorus & more |
| Live Control Surface with physical controls |
| Responsive 7″ LCD Color Touchscreen |
| Intelligent Meters Display Input Level and Fader Volume Position |
| Scene/Preset FX/GEQ: Save, Load, Copy |
| Individual channel delays in 0.2ms increments, up to 300ms for easy sync of video and audio playback |
digiMIX24 FOH and Monitor Mixing
digiMIX24 Virtual Sound Check and Driver Installation
NX Live Performance System with digiMIX24
| Pricing / Images | View |
| Datasheet | DOWNLOAD |
| Manual | DOWNLOAD |
| Module Installation | DOWNLOAD |
| Line Art | DOWNLOAD |
| digiMIX App | DOWNLOAD |
| Dante-32 Interface | View |
| USB Interface | View |
Sound Directions are Dante ™ experts. If you'd like to find out more don't hesitate to get in touch.
