Product Overview
The Walfront ADE-1, ADE-6, and ADE-25 Passive Mixer Modules are engineered for exceptional performance in VHF/UHF applications. Designed to be compact and lightweight, these mixers provide low conversion loss and excellent L-R isolation, making them an ideal choice for RF enthusiasts and professionals alike.
Key Features
- Low Conversion Loss: Achieve optimal performance with conversion losses of 5.0dB (ADE-1), 4.6dB (ADE-6), and 7.0dB (ADE-25).
- Wide Frequency Range: Each model supports different RF/LO frequencies: ADE-1 (0.5-500MHz), ADE-6 (0.05-250MHz), and ADE-25 (5M-2500MHz).
- Compact Design: The mini components design enhances portability and ease of integration into various setups.
- Robust Temperature Range: Operating temperature from -40°C to 85°C ensures reliability in diverse environments.
Technical Specifications
Model | ADE-1 / ADE-6 / ADE-25 |
RF Power | 50mW |
IF Current | 40mA |
Storage Temperature | -55°C to 100°C |
Weight | 9g |
Usage Scenarios
The Passive Mixer Modules are perfect for both hobbyists and professionals looking to build or enhance RF systems. They are excellent for applications requiring high-performance RF signal processing, such as communication systems, signal analyzers, and more.
FAQs
1. What is the primary application of these mixers?
These mixers are designed for VHF/UHF applications, ideal for RF signal processing.
2. How do I choose between ADE-1, ADE-6, and ADE-25?
Select based on your required frequency range: ADE-1 for 0.5-500MHz, ADE-6 for 0.05-250MHz, and ADE-25 for 5M-2500MHz.
3. Are these mixers patented?
Yes, they are protected by US patent 6,133,525, ensuring their unique design and performance.
Originality and Unique Features
What sets the Walfront Passive Mixer Modules apart is not only their compact and lightweight design but also their exceptional low conversion loss and high L-R isolation. These features enhance signal integrity and overall system performance, making them a superior choice for RF applications.
Reviews
There are no reviews yet.