AFS4-09001100-09-S-4

RF Amplifiers Overview

The AFS4-09001100-09-S-4 is an active RF amplifier module manufactured by L3 Narda-MITEQ. It operates within a frequency range of 9 GHz to 11 GHz, designed for GPS applications. The component provides a nominal gain of 32 dB with a P1dB output power of 10 dBm and a noise figure of 0.9 dB. It is housed in a compact module package and requires a 15 V DC supply voltage drawing approximately 100 mA.

RF Amplifiers Feature Summary

• Integrated RF amplification module optimized for high-frequency signal processing
• Low noise figure performance suitable for sensitive receiver front-ends
• Compact module form factor for space-constrained designs

RF Amplifiers Applications

• GPS signal amplification
• Satellite communication systems
• Radar receiver front-ends

RF Amplifiers Procurement Notes

Verify the exact suffix against official L3 Narda-MITEQ documentation to ensure correct pinout and electrical specifications. Confirm RoHS compliance status and lead times directly with authorized distributors or the manufacturer before finalizing procurement plans.

RF Amplifiers Selection Notes

Select this model when a low-noise, moderate-power amplifier is required for the 9-11 GHz band. Compare gain and noise figure requirements against similar AFS series variants to ensure compatibility with system link budgets and impedance matching networks.

RF Amplifiers Part Context

This part belongs to the AFS series of RF amplifier modules from L3 Narda-MITEQ. These modules are engineered for military and aerospace applications requiring reliable performance in harsh environments. The series offers various frequency ranges and gain configurations tailored for specific radar and communication subsystems.

RF Amplifiers Replacement Considerations

Consult official substitution lists for compatible alternatives such as the AFS4-09001100-09-S-4-GW variant. Verify that any substitute maintains identical frequency coverage, gain, and physical footprint to avoid redesigning the host circuit board.