Features:
- Small Size
- Low Power Consumption
- Broad Band
- Low Noise Temperature
Cryogenic Low Noise Amplifiers (LNAs) are specialized electronic devices designed to amplify weak signals with minimal added noise, while operating at extremely low temperatures (typically liquid helium temperatures, 4K or below). These amplifiers are critical in applications where signal integrity and sensitivity are paramount, such as quantumcomputing, radio astronomy, and superconducting electronics. By operating at cryogenic temperatures, LNAs achieve significantly lower noise figures compared to their room-temperature counterparts, making them indispensable in high-precision scientific andtechnological systems.
1. Ultra-Low Noise Figure: Rf cryogenic LNAs achieve noise figures as low as a few tenths of a decibel (dB), which is significantly better than room-temperature amplifiers. This is due to the reduction in thermal noise at cryogenic temperatures.
2. High Gain: Provides high signal amplification (typically 20-40 dB or more) to boost weak signals without degrading the signal-to-noise ratio (SNR).
3. Wide Bandwidth: Supports a broad range of frequencies, from a few MHz to several GHz, depending on the design and application.
4. Cryogenic Compatibility: Microwave cryogenic low noise amplifiers designed to operate reliably at cryogenic temperatures (e.g., 4K, 1K, or even lower). Constructed using materials and components that maintain their electrical andmechanical properties at low temperatures.
5. Low Power Consumption: Optimized for minimal power dissipation to avoid heating the cryogenic environment, which could destabilize the cooling system.
6. Compact and Lightweight Design: Engineered for integration into cryogenic systems, where spaceand weight are often limited.
7. High Linearity: Maintains signal integrity even at high input power levels, ensuring accurateamplification without distortion.
1. Quantum Computing: Millimeter wave cryogenic low noise amplifiers used in superconducting quantum processors to amplify weak readout signals from qubits, enabling accurate measurement of quantum states. Integrated into dilutionrefrigerators to operate at millikelvin temperatures.
2. Radio Astronomy: Employed in cryogenic receivers of radio telescopes to amplify faint signals fromdistant celestial objects, improving the sensitivity and resolution of astronomical observations.
3. Superconducting Electronics: mm wave cryogenic low noise amplifiers used in superconducting circuits and sensors to amplify weak signals while maintaining low noise levels, ensuring accurate signal processing and measurement.
4. Low-Temperature Experiments: Applied in cryogenic research setups, such as studies of superconductivity, quantum phenomena, or dark matter detection, to amplify weak signals withminimal noise.
5. Medical Imaging: Utilized in advanced imaging systems like MRI (Magnetic Resonance Imaging) that operate at cryogenic temperatures to enhance signal quality and resolution.
6. Space and Satellite Communication: Used in cryogenic cooling systems of space-based instruments to amplify weak signals from deep space, improving communication efficiency and data quality.
7. Particle Physics: Employed in cryogenic detectors for experiments such as neutrino detection or dark matter searches, where ultra-low noise amplification is critical.
Qualwave supplies Cryogenic Low Noise Amplifiers from DC to 8GHz, and the noise temperature can be as low as 10K.
Part Number |
Frequency(GHz, Min.) |
Frequency(GHz, Max.) |
Noise Temperature |
P1dB(dBm, Min.) |
Gain(dB, Min.) |
Gain Flatness(±dB, typ.) |
Voltage(VDC) |
VSWR(Max.) |
Lead Time(weeks) |
---|---|---|---|---|---|---|---|---|---|
QCLA-10-2000-35-10 | 0.01 | 2 | 10K | -10 | 35 | - | 1~2 | 1.67 | 2~8 |
QCLA-4000-8000-30-07 | 4 | 8 | 7K | -10 | 30 | - | - | - | 2~8 |
QCLA-4000-8000-40-04 | 4 | 8 | 4K | -10 | 40 | - | - | - | 2~8 |