RCLN1000D-222 Generator is based on diode multipliers that provide ultra-low phase noise

It has additional frequency stabilization achieved using a Phase-Locked Loop (PLL)

And with Temperature-Compensated Crystal Oscillator (TCXO) as a reference,

ensuring high frequency stability over a wide temperature range

Listing includes:

• Ultra Low Noise Reference Oscillator RF Unit [RCLN1000D-222]
• Power Supply [DC 7.5V/2A] [US, EU, UK] [AC plug] (optional, choose in selector)

General information:

RCLN1000D-222 is designed as a high-end reference source for applications requiring utra-low phase noise,
spectral purity, and frequency stability.

This generator is based on diode multipliers that provide ultra-low phase noise.
Additional frequency stabilization is achieved using a Phase-Locked Loop (PLL)
with a Temperature-Compensated Crystal Oscillator (TCXO) as a reference,
ensuring high frequency stability over a wide temperature range.

With an affordable price, ultra-low phase noise, high temperature stability, and excellent noise immunity enabled by its thick aluminum housing
this device stands out as an excellent choice among competing products.

Ideal for use with high-speed digital and mixed-signal systems such as DDS, ADCs, DACs, and other precision RF systems.

When it comes to Direct Digital Synthesizers (DDS), the quality of the output signal is directly determined by the characteristics of the reference clock source.
In RF modules based on the AD9910 and AD9912, using an external low-phase-noise 1 GHz clock generator provides a significant advantage over the internal PLL frequency multipliers integrated within the DDS chips.

These internal PLLs are low-cost compromise solutions — for example, the built-in PLL in both AD9910 and AD9912 typically exhibits a phase noise of around – 115 dBc/Hz at 10 kHz offset – and they introduce a considerable amount of spurious spectral components (spurs), degrading signal purity and preventing the DDS from reaching its full performance potential.

Key parameters of the reference clock source include phase noise (measured in dBc/Hz, where lower is better), frequency stability (in PPM),
as well as minimal harmonic content and absence of spurious signals in the spectrum.
All of these directly affect the output quality of the DDS:
any spectral impurity or noise present in the reference clock will inevitably appear in the output signal spectrum of the synthesizer.

The pursuit of achieving the lowest possible phase noise in a signal generator inevitably leads to increased cost.
That is why we offer our customers a product line that is conditionally divided into two categories:

Base – Low Phase Noise, with typical performance in the range of approximately –136 to –139 dBc/Hz @ 10kHz offset
Premium – Ultra-Low Phase Noise, with performance in the range of –140 to –150 dBc/Hz @ 10kHz offset

Description:

The core of this generator is a specialized Voltage-Controlled Crystal Oscillator (VCXO) operating at 125 MHz with ultra-low phase noise of -168 dBc/Hz at 10 kHz offset.

While VCXOs inherently provide low phase noise, they cannot directly operate at high frequencies without external frequency multipliers. Additionally, they are susceptible to temperature-induced instability— even small temperature variations can cause significant frequency drift. To address these challenges, we implemented three Schottky-diode-based frequency multipliers with intermediate amplification using low-noise monolithic RF amplifiers. Furthermore, we integrated a Phase-Locked Loop (PLL) system with a temperature-compensated crystal oscillator (TCXO) as a reference, achieving precise frequency stabilization via feedback control.

Since PLL systems naturally introduce additional phase noise, we employed an ultra-narrow loop filter bandwidth of just 10 Hz to maintain the VCXO’s low phase noise without adding extraneous noise.

In addition to amplification between the multipliers, a low-noise output amplifier ensures the RCLN1000D-222 delivers a clean output signal at +14 dBm.

Bandpass filters (BPFs) are installed after each amplification stage, including the RCL1000D-222 output, to suppress unwanted harmonics and subharmonics.

To minimize crosstalk between internal modules, the system utilizes five independent power lines, each regulated by a low-dropout (LDO) low-noise voltage regulator,
ensuring minimal phase noise and maximum signal integrity.

The block diagram of this generator is as follows:

Specifications:

• 1 GHz Fixed Frequency
• Low Phase Noise: -150 dBc/Hz @ 20 kHz
• Spurious suppression: < -50 dBc
• Output Power: +14 dBm
• Supply Voltage: 7.5 VDC
• Supply Current: 300 mA
• Operating Temperature: 0°C to +70°C
• Frequency Stability (0-70°С): ±1 ppm (±1 kHz)
• Stability per degree: 0.008 ppm/°C (8 Hz/°C)
• Case Material: Aluminum
• Dimensions: 95х50х31 mm
• Weight: 250 g
• Power Connector: 5.5×2.1 mm (+ in center)
• RF Connector: SMA

We are offering custom design development for this Unit for 1200$.
This comes with condition that at least 10 pieces of them will be ordered then

Applications:

• Frequency Synthesizers (DDS)
• Local Oscillators
• Receivers
• Wireless Communications
• SATCOM
• Optical Communications

Actual Phase Noise Performance:

This graph demonstrates the outstanding phase noise performance of the RCLN1000D-222 generator.
Starting from a 10 kHz offset, the noise level confidently drops below -148 dBc/Hz, reaching -153 dBc/Hz at a 1 MHz offset.
This confirms the exceptional signal quality and makes it a benchmark solution for the most demanding applications.

Spectrograms:

Applications:

Telecommunications:

Low phase noise generators are very important for modern telecommunication systems.
They provide signal stability and accuracy under the conditions of transmitting large volumes of data.
In mobile networks and fiberoptic communication systems frequency control accuracy is needed to prevent interference and ensure high data transmission speeds.
Low phase noise allows for improved communication quality, especially in the high-frequency range, where interference can be particularly noticeable.

Radio Astronomy:

In radio astronomy low phase noise generators are used in radio telescopes to enhance the quality of observations.
This allows for improved accuracy of measurements and the quality of the obtained data.
They are also used in complex systems, such as interferometers, where signals from different antennas need to be precisely synchronized.

Radar:

In radar systems low phase noise generators allow for improved accuracy in determining the distance to objects.
The accuracy of frequency, as well as stability and low noise level, are important when locating objects.
Lower phase noise can lead to more accurate location and identification of objects, especially at long distances.

RCLN1000D-222 Low Noise Reference Oscillator by GRA & AFCH: