Focal Updates the Alpha Evo Studio Monitor Line

Focal Updates the Alpha Evo Studio Monitor Line

Studio Economik |

Focal has updated its Alpha Evo studio monitor line, expanding the series with multiple models designed for music production, recording, and mixing environments. The range includes the Alpha 50 Evo NWG, Alpha 65 Evo NWG, Alpha 80 Evo NWG, and Alpha Twin Evo NWG. Each monitor uses Focal’s aluminium inverted dome tweeter paired with Slatefiber cone woofers developed and manufactured in France. The updated series focuses on consistent tonal balance, wide sound dispersion, and flexible connectivity suited for modern studio setups.

The Alpha Evo NWG monitors share several core design elements across the entire lineup. Each model uses a 25 mm aluminium inverted dome tweeter combined with Slatefiber cone woofers. The Slatefiber material is designed to provide a rigid yet lightweight diaphragm structure, which helps support controlled driver movement and a balanced frequency response. According to the product documentation, this design contributes to sound neutrality while maintaining stable performance at both low and high listening levels.

Connectivity and control options are consistent across the series. Each monitor supports three input types including XLR, TRS, and RCA, allowing users to connect multiple audio sources at the same time. Rear panel controls allow adjustment of sensitivity, mid and low frequency levels, and treble response so the monitors can be adapted to different room conditions and placement scenarios.

The Alpha 50 Evo NWG is the most compact model in the lineup and uses a 5 inch Slatefiber woofer paired with the aluminium tweeter. It includes Class D amplification with 30 W for the low and mid frequencies and 20 W for the high frequencies. The monitor offers a frequency response of 45 Hz to 22 kHz and reaches a maximum peak sound pressure level of 101 dB. This configuration is commonly suited for nearfield monitoring in smaller production spaces.

The Alpha 65 Evo NWG increases the woofer size to 6.5 inches and uses amplification rated at 55 W for the low and mid frequencies and 25 W for the high frequencies. The frequency response extends from 40 Hz to 22 kHz and the monitor reaches a peak SPL of 104 dB. The larger woofer allows for additional low frequency extension while maintaining the same tweeter design and connectivity options found across the series.

The Alpha 80 Evo NWG is designed for situations where higher output levels and deeper bass extension are required. This model uses an 8 inch Slatefiber woofer and includes amplification rated at 80 W for low frequencies and 35 W for high frequencies. Its frequency response extends down to 38 Hz with a peak SPL of 106 dB. These specifications allow the monitor to support monitoring tasks that require extended low frequency detail.

At the top of the range, the Alpha Twin Evo NWG uses a dual 6.5 inch woofer configuration with a centrally positioned aluminium tweeter. Each woofer is powered by its own amplifier delivering 2 × 50 W for low and mid frequencies, while the tweeter uses a 30 W amplifier. The monitor provides a frequency response from 38 Hz to 22 kHz and can reach a peak SPL of 108 dB. Its horizontal cabinet layout allows flexible placement in studio environments while maintaining balanced driver alignment.

The updated Alpha Evo NWG monitors also include practical design features such as an automatic standby mode that activates after approximately fifteen minutes without an audio signal. The cabinets are constructed from 15 mm MDF and use a front laminar port designed to support airflow while reducing turbulence. Several models also include mounting inserts for wall installation when required.

The Alpha Evo NWG lineup provides multiple monitor sizes within a consistent design framework. By offering different woofer configurations and output levels while maintaining the same core driver technologies and connectivity options, the updated series allows users to select a monitor that fits their room size, listening distance, and low frequency requirements.


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