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Potential arrangements of Nooelec SAWBird H1, Nooelec LANA low-noise amplifier, and WT Microwave 1420MHz narrow band cavity filter, to improve radio-astronomy detection of hydrogen line.

Insertion Loss in Nooelec SAWBird H1:

The Nooelec SAWbird+ H1 is a self-contained low-noise amplifier (LNA) module designed for hydrogen line detection around 1420 MHz. It features two ultra-low-noise amplifiers and a custom high-performance surface acoustic wave (SAW) filter centred at the frequency of interest.

The insertion loss of the SAW filter within the SAWbird+ H1 is approximately 2.5dB.

However, the overall module provides a nominal gain of around 40 dB within its passband, effectively compensating for the filter’s insertion loss and amplifying signals in the desired frequency range.

This combination of filtering and amplification makes the SAWbird+ H1 suitable for applications requiring precise frequency selection and signal enhancement, such as hydrogen line observations in radio astronomy.

The Nooelec LANA is a wideband low-noise amplifier (LNA) designed to amplify signals across a broad frequency range. It offers a typical gain of 19dB and a noise figure of approximately 0.6dB. Since the LANA is an amplifier, the concept of insertion loss doesn’t directly apply; instead, it provides signal gain.

Is it possible to compensate for the insertion loss of a cavity RF filter by using an amplifier in front of or behind the cavity RF filter?

It is possible to compensate for the insertion loss of a cavity RF filter by using an amplifier in front of it.

However, there are a few considerations to keep in mind:

Advantages:

  1. Signal Strength Compensation:
    • An amplifier placed before the filter boosts the signal power, compensating for the filter’s insertion loss.
  2. Improved Signal-to-Noise Ratio (SNR):
    • A low-noise amplifier (LNA) in front of the filter can help maintain a better SNR since the noise contribution from the filter will be relatively small compared to the amplified signal.

Considerations:

  1. Nonlinearities:
    • Amplifiers may introduce distortion, intermodulation products, or compression effects, especially if the input signal is strong. Ensure the amplifier operates in its linear range.
  2. Amplifier Noise:
    • The amplifier itself contributes noise, which can degrade the overall system noise figure. Use a low-noise amplifier if SNR is critical.
  3. Filter Selectivity:
    • Placing the amplifier before the filter might amplify out-of-band signals or noise, which could overload the amplifier or subsequent stages. If this is a concern, consider placing the filter first.
  4. Impedance Matching:
    • Ensure proper impedance matching between the amplifier and the filter to minimize signal reflections and maximize power transfer.
  5. Dynamic Range:
    • An amplifier increases the signal level, but it also increases the risk of saturation or overloading downstream components. Ensure the entire system can handle the amplified signal level.

Alternative Configuration:

If your application requires rejecting out-of-band noise or interference, placing the cavity filter before the amplifier might be a better approach. In this case:

  • The filter ensures that only the desired frequency range is amplified.
  • You may need a higher-gain amplifier to compensate for the insertion loss of the filter.

Best Practices:

  • Use a high-quality, low-noise amplifier with sufficient gain and linearity.
  • Evaluate the overall system noise figure, considering the amplifier’s noise figure and the filter’s insertion loss.
  • Test both configurations (amplifier before or after the filter) to determine which performs better for your specific application.

The best configuration for using the Nooelec SAWBird H1, a cavity filter with narrow bandwidth, and possibly a Nooelec LANA depends on your specific application and goals. Below is a recommended setup for a typical use case such as hydrogen line observations in radio astronomy:


Optimal Configuration

  1. Nooelec LANA → Nooelec SAWBird H1 → Receiver:
    • First Stage (Nooelec LANA):
      Use the LANA as a pre-amplifier to boost weak signals before filtering. This ensures that the signal is strong enough to overcome noise introduced by subsequent components.
      • Advantages: Improves the overall system signal-to-noise ratio (SNR) by amplifying the signal before any losses occur in the SAWBird H1.
      • Considerations: Ensure the LANA operates in its linear range and does not saturate due to strong signals or interference.
    • Second Stage (Nooelec SAWBird H1):
      Place the SAWBird H1 (which includes a narrowband filter and additional amplification) after the LANA. This configuration ensures:
      • The cavity filter eliminates out-of-band noise or interference.
      • The internal amplifier in the SAWBird compensates for its own insertion loss and provides additional gain.
      • Advantages: Guarantees that only the desired frequency range (around 1420 MHz) is passed to the receiver.
    • Final Stage (Receiver):
      Connect the output of the SAWBird H1 to your SDR or other receiver for signal processing and analysis.

Why This Configuration Works Well

  • The LANA boosts the weak input signal, which is crucial when dealing with low-power hydrogen line emissions.
  • The SAWBird H1 ensures that only the 1420 MHz hydrogen line signal is passed to the receiver while amplifying it further.
  • This configuration minimizes the impact of:
    • Insertion loss: The LANA compensates for signal loss before filtering.
    • Out-of-band interference: The SAWBird’s SAW filter suppresses undesired frequencies.

Alternative Configuration

If you are in a high-RF interference environment:

  • Place the SAWBird H1 first, followed by the Nooelec LANA:
    • This ensures out-of-band signals are attenuated by the SAWBird’s filter before being amplified by the LANA.
    • Prevents the LANA from being overloaded by strong out-of-band signals.

Final Tips

  1. Power Requirements:
    • Both the LANA and SAWBird H1 need power. Ensure you have a suitable bias tee or power source for both devices.
  2. Impedance Matching:
    • Check the impedance of all components (typically 50 ohms) to ensure proper signal transfer.
  3. Testing:
    • Experiment with both configurations to determine which works best for your environment. RF signal conditions can vary significantly depending on your location.

This configuration provides flexibility while ensuring optimal signal amplification and filtering for hydrogen line detection.

Is there any advantage to adding a cavity filter into the chain, in addition to the Nooelec SAWBird H1 and Nooelec LANA?

Adding a cavity filter to the described setup could provide advantages depending on your specific use case, but it might also introduce redundancy or unnecessary complexity in some scenarios. Here’s an evaluation of whether including a cavity filter adds value:


Advantages of Adding a Cavity Filter

  1. Better Out-of-Band Rejection:
    • A cavity filter has very steep skirts and high Q-factor, which can provide superior out-of-band signal rejection compared to the SAWBird H1’s SAW filter alone.
    • If you are in an RF-rich environment with strong nearby signals (e.g., LTE, Wi-Fi, or other RF noise sources), the cavity filter can provide additional protection against interference.
  2. Prevention of Overload:
    • By attenuating out-of-band signals before they reach the SAWBird H1, the cavity filter reduces the likelihood of saturation or intermodulation distortion in the SAWBird’s internal LNA.
  3. Enhanced Selectivity:
    • A cavity filter can provide more precise frequency selection, ensuring that only signals within the desired narrow bandwidth (e.g., hydrogen line at 1420 MHz) pass through.

Potential Drawbacks

  1. Insertion Loss:
    • Cavity filters typically introduce some insertion loss (e.g., 1-3 dB). If the signal is already weak, this could degrade the signal-to-noise ratio unless compensated with additional amplification.
  2. Redundancy with SAWBird H1:
    • The SAWBird H1 already includes a narrowband SAW filter tuned to 1420 MHz. Adding a cavity filter with a similar passband might not provide significant additional benefit unless the cavity filter has substantially better rejection characteristics.
  3. Increased Complexity:
    • Adding a cavity filter increases the system complexity, requiring additional components, potential impedance matching, and possibly an extra amplifier to offset the cavity filter’s insertion loss.

When to Use a Cavity Filter

  • Yes, use a cavity filter if:
    • You are in an environment with very strong out-of-band interference.
    • You need higher selectivity or better rejection than the SAWBird H1’s SAW filter can provide.
    • Your cavity filter has a significantly narrower or steeper filter response than the SAWBird’s built-in SAW filter.
  • No, skip the cavity filter if:
    • The SAWBird H1’s SAW filter is sufficient for your application’s selectivity and rejection needs.
    • Insertion loss from the cavity filter could degrade the overall system performance.
    • You want to keep the setup simple and avoid redundant components.

Suggested Configuration with a Cavity Filter

If you decide to use a cavity filter:

  1. Configuration:
    LANA → Cavity Filter → SAWBird H1 → Receiver
    • LANA amplifies the weak signal.
    • The cavity filter provides superior out-of-band rejection.
    • The SAWBird H1 performs final filtering and amplification for the 1420 MHz band.
  2. Alternative (High Interference):
    Cavity Filter → LANA → SAWBird H1 → Receiver
    • This ensures that the cavity filter removes interference before it reaches the amplifier, protecting it from overload.

Conclusion

A cavity filter can add value in specific cases where additional out-of-band rejection or higher selectivity is required. However, if the SAWBird H1’s internal SAW filter meets your needs, adding a cavity filter may not provide a significant advantage and could introduce unnecessary loss and complexity.

One thought on “Potential arrangements of Nooelec SAWBird H1, Nooelec LANA low-noise amplifier, and WT Microwave 1420MHz narrow band cavity filter, to improve radio-astronomy detection of hydrogen line.

  • Jerry Taylor

    Do you have any hydrogen data plots showing the various configurations? I would be interested in seeing the impacts of the various configurations on signal strength and noise.

    Thanks!

    Jerry

    Reply

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