ELVA-1 Noise Sources 140 To 330 GHz @Sub-Terahertz-Spectrum

The ISSN-XX noise sources produce a high level of noise power spectral density within the whole waveguide frequency range. These sub-mm-wave sources are available in WR-05 (140-220 GHz) and WR-03 (220-330 GHz) waveguide bands ranges and are based on silicon IMPATT diode which is employed as a fundamental building block of the source. The new…...

See full specification tab below or
Contact us for assistance

At a glance: Key parameters

Product categories: Noise Sources
Manufacturer: Elva-1

The ISSN-XX noise sources produce a high level of noise power spectral density within the whole waveguide frequency range. These sub-mm-wave sources are available in WR-05 (140-220 GHz) and WR-03 (220-330 GHz) waveguide bands ranges and are based on silicon IMPATT diode which is employed as a fundamental building block of the source.

The new devices are intended for test and instrumentation applications in place of gas-tube noise sources. Low DC power requirements eliminate the need for complex high voltage supplies. There are two operation modes: CW mode and pulsed AM mode with modulation frequency up to 1 kHz. Typical value of excess noise ratio (ENR) as a function of frequency is given on the table below.

Parameter: ISSN-05 ISSN-03
Frequency range 140 – 220 GHz 220 – 330 GHz
ENR* 45 dB* 50 dB*
VSWR load 1.5:1 (max) 1.5:1 (max)
Triggering Voltage TTL TTL
Stability, dB/°C 0.025 0.025
Stability, dB/day (typical) 0.05 0.05
Power Supply input Voltage 100 – 240 V AC 50/60 Hz 100 – 240 V AC 50/60 Hz
Waveguide WR-05 WR-03
Flange UG-387/U-M UG-387/U-M
Noise Source biasing Connector BNC-F BNC-F
Noise Source external trigger connector SMA-F SMA-F
Power Supply output Connector BNC-F BNC-F
Weight 3.3 kg (noise source) + 0.6 kg (PSU) 3.3 kg (noise source) + 0.6 kg (PSU)
Operating temperature range 10 to 45 °C 10 to 45 °C
Waveguide flange material Waveguide flange material Waveguide flange material

Noise Sources 140 To 330 GHz @Sub-Terahertz-Spectrum Datasheet

You may also like