TANGO26/0.1M/SMAM/S/RP/29

Antennas RF Overview

The Siretta TANGO26/0.1M/SMAM/S/RP/29 is a passive RF antenna designed for the 2.4 GHz ISM band, specifically covering 2.4 GHz to 2.5 GHz. It features a compact stubby whip design with a 100 mm cable length and an RP-SMA male connector. The unit utilizes surface mount or through-hole mounting options and operates at a nominal impedance of 50 ohms.

Antennas RF Feature Summary

• Compact physical profile suitable for space-constrained wireless device integration
• Integrated low-loss coaxial cable for flexible system layout
• RP-SMA male interface for direct connection to standard wireless modules

Antennas RF Applications

• Wireless LAN (WLAN) devices operating in the 2.4 GHz ISM band
• Bluetooth and BLE enabled consumer electronics
• Industrial IoT sensors requiring reliable short-range connectivity

Antennas RF Procurement Notes

Verify the specific connector polarity variant required by your host board design, as RP-SMA interfaces are distinct from standard SMA. Confirm that the 100 mm cable length aligns with your enclosure constraints. Ensure the mounting method matches your PCB assembly process capabilities.

Antennas RF Selection Notes

Select this component when a low-profile, omnidirectional radiation pattern is required for 2.4 GHz applications. The integrated cable simplifies assembly compared to direct-mount antennas. Consider the mechanical stability provided by the stubby whip form factor in portable or handheld equipment designs.

Antennas RF Part Context

This model belongs to the TANGO series of passive antennas manufactured by Siretta Ltd. The series focuses on providing reliable RF performance for common industrial and commercial wireless standards. The specific designation indicates the cable length, connector type, and mounting configuration.

Antennas RF Replacement Considerations

Direct substitutes include the TANGO25A/0.1M/SMAM/S/RP/29, which shares similar electrical characteristics but may differ in physical dimensions or gain specifications. Verify compatibility with existing RF front-end components before substitution.