SBL-4036032540-1919-E1 ERAVANT | Alldatasheet
Document overview
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Technical content
SBL-4036032540-1919-E1 Rev 1.0 www.eravant.com | 501 Amapola Ave, Torrance, CA 90501 Phone: 424-757-0168 | Fax: 424-757-0188 | Email: support@eravant.com Page | 1 SAGE Millimeter, Inc. U-Band Low Noise Amplifier, 40 to 60 GHz, 25 dB Gain, 4.0 dB NF Copyright © 2022 by Eravant Description: Model SBL-4036032540-1919-E1 is a low noise amplifier with a typical small signal gain of 25 dB across the frequency range of 40 to 60 GHz and a nominal noise figure of 4.0 dB. The DC power requirement for the amplifier is +8 VDC/60 mA. The mechanical configuration offers an in-line structure WR-19 Uni-Guide™ waveguides. Other port configurations, such as a right angle structure with WR-19 waveguides or 1.85 mm connectors, are also available under different model numbers. Features:
- Full Waveguide Band Operations
- State-of-the-Art Noise Figure Applications:
- New 5G Bands
- Low Noise Receivers
- Communication Systems
- Radar Systems Electrical Specifications: Parameter Minimum Typical Maximum Frequency 40 GHz 60 GHz Gain 25 dB Noise Figure 4.0 dB P1dB 0 dBm Pin +15 dBm Input Return Loss 8 dB Output Return Loss 10 dB DC Voltage +6 VDC +8 VDC +15 VDC DC Supply Current 60 mA Specification Temperature +25 ˚C Operating Temperature 0 ˚C +50 ˚C Mechanical Specifications: Item Specification RF Ports WR-19 Uni-Guide™ Waveguides with UG-383/U-M Anti-Cocking Flanges Bias Solder Pin Case Material Aluminum Finish Gold Plated Weight 2.0 Oz Outline BG-SU-2-A
SBL-4036032540-1919-E1 Rev 1.0 www.eravant.com | 501 Amapola Ave, Torrance, CA 90501 Phone: 424-757-0168 | Fax: 424-757-0188 | Email: support@eravant.com Page | 2 SAGE Millimeter, Inc. U-Band Low Noise Amplifier, 40 to 60 GHz, 25 dB Gain, 4.0 dB NF Copyright © 2022 by Eravant -30.00 -20.00 -10.00 0.00 10.00 20.00 30.00 -30.00 -20.00 -10.00 0.00 10.00 20.00 30.00 40 42 44 46 48 50 52 54 56 58 60 Return Loss (dB) Gain (dB) Frequency (GHz) Gain and Return Loss vs. Frequency Bias: +8 VDC/65mA Gain Input Return Loss Output Return Loss 40 42 44 46 48 50 52 54 56 58 60 Noise Figure (dB) Frequency (GHz) Noise Figure vs. Frequency Bias: +8 VDC/65mA
SBL-4036032540-1919-E1 Rev 1.0 www.eravant.com | 501 Amapola Ave, Torrance, CA 90501 Phone: 424-757-0168 | Fax: 424-757-0188 | Email: support@eravant.com Page | 3 SAGE Millimeter, Inc. U-Band Low Noise Amplifier, 40 to 60 GHz, 25 dB Gain, 4.0 dB NF Copyright © 2022 by Eravant Mechanical Outline: (Unless otherwise specified, all dimensions are in inches [millimeters]) 40 42 44 46 48 50 52 54 56 58 60 P1dB (dBm) Frequency (GHz) P1dB vs. Frequency Bias: +8VDC/67mA
SBL-4036032540-1919-E1 Rev 1.0 www.eravant.com | 501 Amapola Ave, Torrance, CA 90501 Phone: 424-757-0168 | Fax: 424-757-0188 | Email: support@eravant.com Page | 4 SAGE Millimeter, Inc. U-Band Low Noise Amplifier, 40 to 60 GHz, 25 dB Gain, 4.0 dB NF Copyright © 2022 by Eravant Note:
- All data presented is collected from a sample lot. Actual data may vary unit to unit.
- All testing was performed under +25 ˚C case temperature.
- The amplifier employs SAGE Millimeter’s trademarked and patent pending technology, the Uni- GuideTM, as its waveguide interfaces. The orientation of the input and the output waveguides can be specified through corresponding model numbers. For example, the model number for a vertical input waveguide and horizontal output waveguide configuration would be SBL- 4036032540-1919H-E1 instead of the default SBL-4036032540-1919-E1 which indicates vertical orientation for both input and output.
- Other mechanical configurations are available under different model numbers.
- Eravant reserves the right to change the information presented without notice. Caution:
- Exceeding absolute maximum ratings shown will damage the device.
- The device is static sensitive. Always follow ESD rules when working with the device.
- The case temperature of the device shall never exceed +50 ˚C. Use proper heatsink or fan if necessary.
- Any foreign objects in the waveguide will cause performance degradation and may damage the device.