LNA-30-00100400-13-10P

Overview

The LNA-30-00100400-13-10P is a low-noise amplifier module from L3 Narda-MITEQ designed for VSAT applications. It operates within a frequency range of 100 MHz to 4 GHz. The device provides a nominal gain of 30 dB with a typical noise figure of 1.3 dB. It features an output power level (P1dB) of 10 dBm and requires a +15 VDC supply voltage. The unit utilizes SMA connectors for input and output interfaces and is housed in a compact module package.

Feature Summary

• Provides stable signal amplification across the 100 MHz to 4 GHz frequency spectrum
• Engineered for high sensitivity reception in satellite communication systems
• Features standard 50 Ohm impedance matching for seamless system integration

Applications

• VSAT satellite communication ground station receivers
• RF signal conditioning in microwave link systems
• Test and measurement instrumentation front-ends

Procurement Notes

Verify the specific datasheet revision and manufacturing lot date code upon order confirmation. Confirm that the SMA connector polarity and module pinout align with your PCB layout requirements. Ensure the +15 VDC power supply specifications meet the current consumption limits defined in the official electrical characteristics table to guarantee reliable operation.

Selection Notes

Select this component when a wideband low-noise solution is required for frequencies up to 4 GHz. It is suitable for designs prioritizing moderate gain and low noise figure in space-constrained modules. Consider thermal management capabilities if operating at the upper temperature limits specified in the datasheet.

Part Context

This part belongs to the LNA-30 series of low-noise amplifiers manufactured by L3 Narda-MITEQ, now part of L3Harris Technologies. The series is characterized by ruggedized module construction and consistent RF performance for defense and commercial satellite communications.

Replacement Considerations

Consult official cross-reference lists for direct substitutes. Alternative models may offer different frequency ranges or gain profiles. Verify compatibility with existing biasing networks and mechanical mounting constraints before substitution.