Products> Antenna Products > Cassegrain Antennas
Mi-Wave’s Series 222 and Series 223 Cassegrain Reflector Antennas are high-performance directional antennas engineered to deliver high gain, narrow beamwidth, and efficient feed integration across RF, microwave, and millimeter-wave frequency ranges. These antennas use a dual-reflector Cassegrain configuration that combines a primary parabolic reflector with a secondary hyperbolic sub-reflector, allowing RF energy to be focused efficiently while keeping the feed assembly closer to the rear of the antenna structure.
This design helps reduce front-aperture blockage, simplifies feed and waveguide integration, and supports more compact system layouts compared to many conventional reflector antenna configurations. By improving feed placement and maintaining controlled reflector geometry, Cassegrain antennas provide stable radiation patterns, predictable beam performance, and efficient use of aperture area.
Mi-Wave Cassegrain antennas are well suited for communications, radar, telemetry, satellite tracking, antenna test ranges, and research systems where precise beam control and repeatable electrical performance are important. Standard configurations support operation from 5.0 GHz to 110 GHz with reflector diameters from 10 inches to 48 inches, depending on frequency, gain requirements, and mechanical configuration.
The 222 Series uses aluminum reflector construction, providing a rigid and mechanically stable antenna structure with excellent surface accuracy and electrical performance. This makes the 222 Series well suited for laboratory systems, fixed installations, antenna measurement ranges, radar calibration, and applications where dimensional stability is critical.
The 223 Series uses metallized fiberglass reflector construction for lighter-weight antenna structures. This option is useful in applications where reduced mass, environmental durability, and long-term outdoor performance are important, while still maintaining reliable RF performance across the intended operating band.
MI-Wave also notes that many additional custom Cassegrain configurations are available beyond the standard models shown online, including variations in diameter, frequency range, polarization, feed arrangement, and mounting.
Outlines & Drawings
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| Model No. | Waveguide Band | Reflector diameter (inches) | Circular Waveguide Internal Diameter (.XXX in Model No.) in Inches | Frequency Range (GHz) | Gain (dB) | 3 dB Beamwidth (degree) | Polarization | VSWR | Antenna Port | Reflector material |
|---|---|---|---|---|---|---|---|---|---|---|
| 222X-18/.XXX/39 and 223X-18/.XXX/39 | X-band | 18 | .XXX=1.094 .XXX=.938 .XXX= .797 | 8.2-9.97 8.5-11.6 9.97-12.4 | 29 | 4.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-39/U Flange | Aluminum/Fibreglass |
| 222X-24/.XXX/39 and 223X-24/.XXX/39 | X-band | 24 | .XXX=1.094 .XXX=.938 .XXX= .797 | 8.2-9.97 8.5-11.6 9.97-12.4 | 32 | 3.5 | Circular Polarized | 1.3:1 | Cicular Waveguide with UG-39/U Flange | Aluminum/Fibreglass |
| 222Ku-18/.XXX/419 and 223-18/.XXX/419 | Ku-Band | 18 | XXX=.660 XXX=.550 | 12.4-14.6 14.6-18 | 33 | 3 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-419/U Flange | Aluminum/Fibreglass |
| 222Ku-24/.XXX/419 and 223-24/.XXX/419 | Ku-Band | 24 | XXX=.660 XXX=.550 | 12.4-14.6 14.6-18 | 36.5 | 2 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-419/U Flange | Aluminum/Fibreglass |
| 223Ku-36/.XXX/419 | Ku-Band | 36 | XXX=.660 XXX=.550 | 12.4-14.6 14.6-18 | 40.5 | 1.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-419/U Flange | Fibreglass |
| 223Ku-48/.XXX/419 | Ku-Band | 48 | XXX=.660 XXX=.550 | 12.4-14.6 14.6-18 | 43 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-419/U Flange | Fibreglass |
| 222K-18/.XXX/595 and 223K-18/.XXX/595 | K-Band | 18 | XXX=.470 XXX .396 XXX=.328 | 18-20.5 20.4-24.5 24.5-26.5 | 36 | 2 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-595/U Flange or UG-425/U Flange | Aluminum/Fibreglass |
| 222K-24/.XXX/595 and 223K-24/.XXX/595 | K-Band | 24 | XXX=.470 XXX .396 XXX=.328 | 18-20.5 20.4-24.5 24.5-26.5 | 39 | 1.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-595/U Flange or UG-425/U Flange | Aluminum/Fibreglass |
| 223K-36/.XXX/595 | K-Band | 36 | XXX=.470 XXX .396 XXX=.328 | 18-20.5 20.4-24.5 24.5-26.5 | 43 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-595/U Flange or UG-425/U Flange | Fibreglass |
| 223K-48/.XXX/595 | K-Band | 48 | XXX=.470 XXX .396 XXX=.328 | 18-20.5 20.4-24.5 24.5-26.5 | 45.5 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-595/U Flange or UG-425/U Flange | Fibreglass |
| 222A-18/.XXX/599 and 223A-18/.XXX/599 | Ka-Band | 18 | XXX=.328 XXX=.281 XXX=.250 XXX= .219 | 26.5-28.5 28.5-33.0 33.0 -38.5 38.5-40.0 | 39 | 1.3 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-599/U Flange or UG-381/U Flange | Aluminum/Fibreglass |
| 222A-24/.XXX/599 and 223A-24/.XXX/599 | Ka-Band | 24 | XXX=.328 XXX=.281 XXX=.250 XXX= .219 | 26.5-28.5 28.5-33.0 33.0 -38.5 38.5-40.0 | 42 | 1.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-599/U Flange or UG-381/U | Aluminum/Fibreglass |
| 223A-36/.XXX/599 | Ka-Band | 36 | XXX=.328 XXX=.281 XXX=.250 XXX= .219 | 26.5-28.5 28.5-33.0 33.0 -38.5 38.5-40.0 | 45.5 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-599/U Flange or UG-381/U | Fibreglass |
| 223A-48/.XXX/599 | Ka-Band | 48 | XXX=.328 XXX=.281 XXX=.250 XXX= .219 | 26.5-28.5 28.5-33.0 33.0 -38.5 38.5-40.0 | 48 | 0.8 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-599/U Flange or UG-381/U | Fibreglass |
| 222B-18/.XXX/383 and 223B-18/.XXX/383 | B-Band | 18 | XXX=.250 XXX=.219 XXX=.188 | 33.0-38.5 38.5-43.0 43.0-50.0 | 42 | 1.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U Flange | Aluminum/Fibreglass |
| 222B-24/.XXX/383 and 223B-24/.XXX/383 | B-Band | 24 | XXX=.250 XXX=.219 XXX=.188 | 33.0-38.5 38.5-43.0 43.0-50.0 | 44 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U Flange | Aluminum/Fibreglass |
| 223B-36/.XXX/383 | B-Band | 36 | XXX=.250 XXX=.219 XXX=.188 | 33.0-38.5 38.5-43.0 43.0-50.0 | 48 | 0.7 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U Flange | Fibreglass |
| 223B-48/.XXX/383 | B-Band | 48 | XXX=.250 XXX=.219 XXX=.188 | 33.0-38.5 38.5-43.0 43.0-50.0 | 50 | 0.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U Flange | Fibreglass |
| 222U-18/.XXX/383 and 223U-18/.XXX/383 | U-Band | 18 | XXX=.219 XXX=.188 XXX=.165 XXX=.141 | 38.5-43.0 43.0-50.0 50.0-58.0 58.0-60.0 | 43 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U-M Flange | Aluminum/Fibreglass |
| 222U-24/.XXX/383 and 223U-24/.XXX/383 | U-Band | 24 | XXX=.219 XXX=.188 XXX=.165 XXX=.141 | 38.5-43.0 43.0-50.0 50.0-58.0 58.0-60.0 | 46 | 0.7 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U-M Flange | Aluminum/Fibreglass |
| 223U-36/.XXX/383 | U-Band | 36 | XXX=.219 XXX=.188 XXX=.165 XXX=.141 | 38.5-43.0 43.0-50.0 50.0-58.0 58.0-60.0 | 49.5 | 0.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U-M Flange | Fibreglass |
| 223U-48/.XXX/383 | U-Band | 48 | XXX=.219 XXX=.188 XXX=.165 XXX=.141 | 38.5-43.0 43.0-50.0 50.0-58.0 58.0-60.0 | 52 | 0.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-383/U-M Flange | Fibreglass |
| 222V-12/.XXX/385 and 223V-12/.XXX/385 | V-Band | 12 | XXX=.165 XXX=.141 XXX=.125 | 50.0-58.0 58.0-68.0 68.0-75.0 | 42 | 1.2 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-385/U Flange | Aluminum/Fibreglass |
| 222V-18/.XXX/385 and 223V-18/.XXX/385 | V-Band | 18 | XXX=.165 XXX=.141 XXX=.125 | 50.0-58.0 58.0-68.0 68.0-75.0 | 45 | 0.9 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-385/U Flange | Aluminum/Fibreglass |
| 222V-24/.XXX/385 and 223V-24/.XXX/385 | V-Band | 24 | XXX=.165 XXX=.141 XXX=.125 | 50.0-58.0 58.0-68.0 68.0-75.0 | 58 | 0.6 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-385/U Flange | Aluminum/Fibreglass |
| 223V-36/.XXX385 | V-Band | 36 | XXX=.165 XXX=.141 XXX=.125 | 50.0-58.0 58.0-68.0 68.0-75.0 | 51 | 0.4 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-385/U Flange | Fibreglass |
| 223V-48/385 | V-Band | 48 | XXX=.165 XXX=.141 XXX=.125 | 50.0-58.0 58.0-68.0 68.0-75.0 | 54 | 0.3 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-385/U Flange | Fibreglass |
| 222E-12/.XXX/387 and 223E-12/.XXX/387 | E-Band | 12 | XXX=.141 XXX=.125 XXX=.110 XXX=.094 | 60.0-68.0 68.0-77.0 77.0-87.0 87.0-90.0 | 43 | 1 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U Flange | Aluminum/Fibreglass |
| 222E-18/.XXX/387 and 223E-18/.XXX/387 | E-Band | 18 | XXX=.141 XXX=.125 XXX=.110 XXX=.094 | 60.0-68.0 68.0-77.0 77.0-87.0 87.0-90.0 | 47 | 0.6 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U Flange | Aluminum/Fibreglass |
| 222E-24/.XXX/387 and 223E-24/.XXX/387 | E-Band | 24 | XXX=.141 XXX=.125 XXX=.110 XXX=.094 | 60.0-68.0 68.0-77.0 77.0-87.0 87.0-90.0 | 49 | 0.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U Flange | Aluminum/Fibreglass |
| 223E-36/.XXX/387 | E-Band | 36 | XXX=.141 XXX=.125 XXX=.110 XXX=.094 | 60.0-68.0 68.0-77.0 77.0-87.0 87.0-90.0 | 56 | 0.35 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U Flange | Fibreglass |
| 223E-48/.XXX/387 | E-Band | 48 | XXX=.141 XXX=.125 XXX=.110 XXX=.094 | 60.0-68.0 68.0-77.0 77.0-87.0 87.0-90.0 | 55.5 | 0.3 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U Flange | Fibreglass |
| 222W-12/.XXX/387 and 223W-12/.XXX/387 | W-Band | 12 | XXX=.125 XXX=.110 XXX=.094 XXX=.082 | 75.0-77.0 77.0-87.0 87.0-100.0 100.0-110.0 | 45 | 0.8 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U-M Flange | Aluminum/Fibreglass |
| 222W-18/.XXX/387 and 223W-18/.XXX/387 | W-Band | 18 | XXX=.125 XXX=.110 XXX=.094 XXX=.082 | 75.0-77.0 77.0-87.0 87.0-100.0 100.0-110.0 | 49 | 0.5 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U-M Flange | Aluminum/Fibreglass |
| 222W-24/.XXX/387 and 203W-24/.XXX/387 | W-Band | 24 | XXX=.125 XXX=.110 XXX=.094 XXX=.082 | 75.0-77.0 77.0-87.0 87.0-100.0 100.0-110.0 | 51 | 0.4 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U-M Flange | Aluminum/Fibreglass |
| 223W-36/.XXX/387 | W-Band | 36 | XXX=.125 XXX=.110 XXX=.094 XXX=.082 | 75.0-77.0 77.0-87.0 87.0-100.0 100.0-110.0 | 55 | 0.25 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U-M Flange | Fibreglass |
| 223W-48/.XXX/387 | W-Band | 48 | XXX=.125 XXX=.110 XXX=.094 XXX=.082 | 75.0-77.0 77.0-87.0 87.0-100.0 100.0-110.0 | 57 | 0.18 | Circular Polarized | 1.3:1 | Circular Waveguide with UG-387/U-M Flange | Fibreglass |
*All data presented is collected from a sample lot.
* Actual data may vary unit to unit, slightly.
*All testing was performed under +25 °C case temperature.
*Consult factory to confirm if material, plating, size, shape, orientation and any electrical parameter is critical for the application as website information is for reference only.
*Millimeter Wave Products, Inc. reserves the right to change the information presented on website without notice as we continue to enhance the performance and design of our products.
Key Features & Performance Benefits
High Gain Performance
Cassegrain reflector antennas deliver strong directional gain across RF, microwave, and millimeter-wave frequencies. Their dual-reflector geometry helps concentrate energy efficiently, making them well suited for long-range communication links, radar systems, and precision measurement applications.
Narrow Beamwidth
The high directivity of a Cassegrain antenna produces narrow beamwidths for accurate pointing, improved target resolution, and reduced off-axis interference. This is especially valuable in satellite tracking, radar testing, and antenna range environments.
Compact Feed Integration
The Cassegrain design places the feed closer to the main reflector structure, creating a more compact and practical system layout. This configuration simplifies integration of feeds, waveguide components, and RF hardware while supporting high-frequency operation.
Efficient Dual-Reflector Design
By using both a main reflector and a sub-reflector, Cassegrain antennas can improve illumination efficiency and support strong overall aperture performance. This helps maximize gain while maintaining predictable beam characteristics.
Stable Radiation Patterns
Cassegrain antennas are designed to provide repeatable and controlled radiation performance across their intended operating bands. This makes them ideal for applications where beam shape, sidelobe behavior, and measurement consistency are critical.
Broad Frequency Coverage
Available across wide RF, microwave, and millimeter-wave frequency ranges, Cassegrain antennas support applications from lower microwave bands through Ka, Q, V, and W-Band systems. Their versatility makes them suitable for both commercial and defense-related platforms.
Precision Measurement Capability
These antennas are widely used in antenna test ranges, calibration systems, and laboratory environments where accurate gain, beamwidth, and pattern measurements are required. Their predictable directional performance supports reliable RF testing and validation.
Multiple Reflector Construction Options
Cassegrain antennas are available in different reflector materials, including aluminum and lightweight fiberglass configurations, allowing engineers to balance performance, structural requirements, and environmental needs.
Custom Configurations Available
Custom diameters, feeds, frequency ranges, polarization schemes, and mounting arrangements can be developed for specialized applications. This flexibility supports mission-specific requirements in communications, radar, research, and system integration projects.
Well Suited for High-Frequency Systems
Cassegrain reflector antennas perform particularly well in microwave and millimeter-wave environments where compact feed layouts, high gain, and tight beam control are essential. They are a strong fit for advanced satcom, radar, and test systems.
How Cassegrain Antennas Work & How to Select the Right Antenna
Cassegrain reflector antennas are high-gain directional antennas that use a dual-reflector architecture to improve feed integration, reduce feed blockage, and support compact high-performance RF, microwave, and millimeter-wave systems.
How Cassegrain Antennas Work
A Cassegrain antenna uses two reflector surfaces to focus and direct electromagnetic energy. The primary reflector is a parabolic dish, while the secondary reflector is typically hyperbolic and positioned between the main reflector and the feed system.
Incoming RF energy first reflects from the main parabolic reflector toward the secondary sub-reflector, which redirects the energy into the feed assembly located behind the primary reflector.
During transmission, the process operates in reverse. RF energy from the feed illuminates the secondary reflector, which distributes the energy onto the primary reflector to form a narrow high-gain beam.
Why the Dual-Reflector Design Matters
The Cassegrain configuration improves feed placement and reduces feed-line obstruction compared to conventional prime focus reflector systems.
Positioning the feed closer to the rear of the antenna can simplify RF integration, reduce feed support blockage, shorten waveguide runs, and improve overall system packaging.
This design is especially valuable in radar, satellite communication, telemetry, and high-frequency microwave systems.
High Gain & Beam Control
Cassegrain antennas provide high directivity and narrow beamwidth by efficiently concentrating RF energy into a focused radiation pattern.
Larger reflector diameters generally provide:
- Higher antenna gain
- Narrower beamwidth
- Improved pointing accuracy
- Greater long-range communication performance
Frequency Range Considerations
Mi-Wave Series 222 and 223 Cassegrain antennas support operation from approximately 5 GHz to 110 GHz depending on reflector size, surface accuracy, and feed configuration.
At microwave and millimeter-wave frequencies, reflector precision becomes increasingly important because small surface variations can affect gain, sidelobe levels, and beam symmetry.
Choosing Reflector Diameter
Reflector diameter directly affects antenna performance. Larger antennas provide higher gain and narrower beamwidth but require more installation space and tighter mechanical alignment.
Engineers typically balance:
- Operating frequency
- Required gain
- Beamwidth objectives
- Mechanical constraints
- Environmental exposure
Aluminum vs Fiberglass Reflectors
The 222 Series uses aluminum reflector construction for rigid mechanical stability, excellent conductivity, and precise surface accuracy.
The 223 Series utilizes metallized fiberglass reflectors to reduce antenna weight while maintaining reliable RF performance. These lighter-weight structures are useful in applications where reduced mass or environmental durability is important.
Feed Integration & Waveguide Interfaces
Cassegrain antennas commonly integrate with horn feeds, OMTs, scalar feeds, LNAs, HPAs, and standard WR-series waveguide interfaces depending on system requirements.
Proper feed alignment and impedance matching help optimize aperture efficiency, polarization purity, and sidelobe performance.
Polarization Considerations
Cassegrain systems may support linear or circular polarization depending on the feed architecture and communication requirements.
Stable polarization performance is critical in satellite communication systems, radar applications, and dual-polarized microwave links.
Environmental & Mechanical Factors
Outdoor and high-frequency systems may require additional consideration for wind loading, vibration, thermal expansion, corrosion resistance, and long-term environmental stability.
Mechanical alignment becomes increasingly important as operating frequency increases into millimeter-wave bands.
Custom Cassegrain Configurations
In addition to standard models, custom Cassegrain reflector configurations may include:
- Custom reflector diameters
- Extended frequency coverage
- Specialized feed systems
- Custom mounting arrangements
- Linear or circular polarization
- Integrated RF subsystems
These configurations support specialized communication, radar, aerospace, and research applications.
Common Applications
Cassegrain reflector antennas are widely used in:
- Satellite communications
- Radar systems
- Telemetry tracking
- Test ranges
- Microwave communication links
- Research laboratories
- Millimeter-wave measurement systems
Cassegrain Antenna Engineering Calculators
These RF engineering calculators help estimate antenna performance for Cassegrain reflector antennas, including satcom systems, radar platforms, antenna measurement ranges, and millimeter-wave test environments. Use them to calculate antenna gain, beamwidth, reflector diameter required for target gain, effective aperture, free-space path loss, and wavelength across RF, microwave, and millimeter-wave frequencies.
Cassegrain antennas use a dual-reflector design, so efficiency is often slightly higher than prime focus designs. For many systems, a typical starting efficiency range is 0.55 to 0.75.
Antenna Gain Calculator
Antenna Gain (dBi):
Antenna Beamwidth Calculator
Reflector Size Required for Target Gain
Antenna Effective Aperture Calculator
Effective Aperture (m²):
Free Space Path Loss Calculator
RF Wavelength Calculator
Wavelength (mm):
Applications
Mi-Wave Prime Focus Antennas are widely used across RF, microwave, and millimeter-wave systems that require high-gain directional antennas, predictable radiation patterns, and stable performance across wide frequency ranges. Their precision reflector geometry and controlled beam characteristics make them ideal for both communication systems and RF measurement environments.
These antennas support applications in satellite communications, radar systems, antenna measurement ranges, wireless research, and electromagnetic compatibility testing, where accurate signal transmission and reception are essential.
Satellite Communications (SatCom)
Prime focus antennas are commonly used in satellite communication systems for both uplink and downlink operations. Their high gain and narrow beamwidth allow efficient communication with satellites operating in microwave and millimeter-wave frequency bands.
Typical satcom applications include:
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Satellite ground terminals and gateway stations
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Experimental satellite communication links
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Ka-band, Q-band, and V-band research systems
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Telemetry and satellite tracking systems
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Antenna testing for satcom payload development
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RF link experiments and satellite communication demonstrations
These antennas help provide stable beam patterns and high signal gain, improving link reliability and signal quality in satellite communication environments.
Antenna Measurement Ranges
Prime focus antennas are widely used in antenna measurement facilities where accurate radiation pattern characterization and gain measurements are required.
Typical measurement applications include:
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Antenna gain and pattern measurements
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Near-field and far-field antenna testing
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Calibration of RF antennas and measurement equipment
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Verification of antenna beamwidth and sidelobe levels
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RF component and subsystem testing
The predictable radiation pattern of prime focus reflectors makes them well suited for precision RF measurement and calibration environments.
Radar Testing and Radar Systems
Prime focus antennas are often integrated into radar research and radar testing platforms where high directivity and stable beam patterns are required.
Common radar applications include:
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Radar cross-section (RCS) testing
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Radar signal transmission and reception
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Radar calibration and system verification
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FMCW and pulse radar research systems
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Microwave and millimeter-wave radar experiments
Their high gain and directional characteristics allow radar engineers to control signal illumination and improve measurement accuracy.
RF and Microwave Laboratory Research
Research laboratories and universities frequently use prime focus antennas in RF and microwave experimental systems for signal transmission, propagation studies, and antenna research.
Typical research applications include:
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Wireless propagation experiments
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Microwave and millimeter-wave system development
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RF component characterization
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Advanced antenna design research
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Academic and government research projects
These antennas provide a stable and repeatable RF platform for experimental testing and system prototyping.
EMC and RF Test Facilities
Prime focus antennas are also used in electromagnetic compatibility (EMC) testing environments where controlled radiation patterns and directional signal transmission are required.
Common EMC applications include:
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Radiated emissions testing
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RF susceptibility testing
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Controlled RF illumination in test chambers
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EMC measurement and compliance verification
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Antenna system validation
Their directional performance allows engineers to focus RF energy toward specific test targets, improving measurement precision.
Frequently Asked Questions (FAQ)
What is a Cassegrain antenna?
A Cassegrain antenna is a dual-reflector antenna that uses a primary parabolic reflector and a secondary sub-reflector to direct RF energy between the feed and the main dish. This design supports high gain, narrow beamwidth, and compact feed placement.
What are the advantages of a Cassegrain antenna?
Cassegrain antennas offer high directional gain, compact feed integration, narrow beamwidth, and efficient reflector illumination. They are often chosen for systems that need strong performance at microwave and millimeter-wave frequencies while keeping the feed arrangement closer to the antenna structure.
What is the difference between a Cassegrain antenna and a prime focus antenna?
A prime focus antenna places the feed directly at the focal point of the main reflector, while a Cassegrain antenna uses a secondary reflector to redirect energy between the feed and the main reflector. Cassegrain designs can offer more compact packaging and improved feed placement, while prime focus designs are simpler.
What frequencies do Cassegrain antennas support?
Cassegrain antennas can support a wide range of RF, microwave, and millimeter-wave frequencies, depending on reflector size, feed design, and surface accuracy. They are commonly used in X, Ku, K, Ka, Q, V, and W-Band systems.
What determines antenna gain in a Cassegrain antenna?
Antenna gain is primarily determined by reflector diameter, operating frequency, aperture efficiency, and feed illumination quality. Larger reflectors and higher frequencies typically produce higher gain and narrower beamwidth.
Why are Cassegrain antennas often used at high frequencies?
Cassegrain antennas are well suited for higher-frequency systems because their design supports tight beam control, efficient feed integration, and compact placement of RF hardware. These benefits are especially useful in microwave and millimeter-wave applications.
What is beamwidth in a Cassegrain antenna?
Beamwidth is the angular width of the main radiation beam. In Cassegrain antennas, beamwidth decreases as reflector diameter increases or wavelength decreases, allowing for highly directional performance.
What is antenna efficiency in a Cassegrain antenna?
Antenna efficiency describes how effectively the antenna converts input RF power into useful radiated or received energy. In Cassegrain systems, efficiency is influenced by reflector illumination, spillover, blockage, alignment, and surface accuracy.
What are Cassegrain antennas used for?
Cassegrain antennas are commonly used in:
- Satellite communications (SatCom)
- Radar systems
- Antenna measurement ranges
- RF and microwave laboratories
- Telemetry and tracking systems
- EMC and RF test environments
- Millimeter-wave research platforms
Are Cassegrain antennas suitable for test and measurement applications?
Yes. Their high gain, stable radiation patterns, and narrow beamwidth make them well suited for antenna testing, calibration, pattern measurement, and high-frequency RF evaluation.
Can Cassegrain antennas be customized?
Yes. Cassegrain antennas can be customized for diameter, frequency range, feed type, polarization, mounting configuration, reflector material, and environmental requirements.
What materials are used in Cassegrain antennas?
Cassegrain antennas are often available in aluminum and fiberglass reflector constructions, depending on system weight, stiffness, environmental exposure, and frequency requirements.
What is a sub-reflector in a Cassegrain antenna?
The sub-reflector is the secondary reflector positioned between the main reflector and the feed. It redirects RF energy so the feed can be placed closer to the rear or center of the antenna structure.
Why is feed placement important in a Cassegrain antenna?
Feed placement affects mechanical packaging, RF performance, integration with waveguide or coax components, and overall system layout. One advantage of the Cassegrain design is that it allows a more compact feed arrangement than many prime focus designs.
Glossary of Cassegrain Antenna Terms
This glossary defines key terminology related to Cassegrain reflector antennas used in RF, microwave, and millimeter-wave systems. These antennas are commonly used in satellite communications, radar, antenna measurement ranges, RF laboratories, telemetry systems, and research environments where high gain, narrow beamwidth, and compact feed integration are important.
Reflector Antenna Fundamentals
Cassegrain Antenna
A dual-reflector antenna design that uses a main parabolic reflector and a secondary sub-reflector to direct RF energy between the feed and the main dish.
Primary Reflector
The main parabolic reflector surface that shapes and directs the antenna’s radiation pattern.
Sub-Reflector
The secondary reflector used to redirect RF energy between the feed and the primary reflector.
Parabolic Reflector
A curved reflector surface shaped to focus electromagnetic energy toward a focal region.
Reflector Diameter
The physical width of the main reflector. Larger diameters generally provide higher gain and narrower beamwidth.
Reflector Aperture
The effective opening area of the reflector that captures or radiates RF energy.
Reflector Surface Accuracy
The degree to which the reflector surface matches the intended geometry. Higher accuracy is especially important at microwave and millimeter-wave frequencies.
Reflector Rim
The outer edge of the reflector that defines its physical boundary.
Feed System Terms
Feed Antenna
The radiating element that launches or receives RF energy within the reflector system.
Feed Placement
The physical location of the feed relative to the reflector system. In a Cassegrain antenna, the feed is positioned so it works through the sub-reflector rather than illuminating only the main reflector directly.
Horn Feed
A horn antenna commonly used as the feed because of its controlled radiation pattern and broadband RF performance.
Feed Illumination Pattern
The distribution of RF energy from the feed across the reflector system.
Edge Taper
The reduction in feed illumination toward the reflector edge to reduce sidelobes and spillover.
Feed Blockage
Loss caused when the feed or support structure blocks part of the reflector aperture.
Spillover
RF energy that misses the intended reflector surfaces and does not contribute to useful radiation.
Feed Support Structure
The mechanical structure that holds the feed and, in some cases, the sub-reflector in the correct position.
Radiation and Performance Terms
Antenna Gain
A measure of how effectively an antenna concentrates RF energy in a given direction relative to an isotropic source.
Directivity
The degree to which radiation is focused in a preferred direction.
Beamwidth
The angular width of the main radiation lobe.
Half-Power Beamwidth (HPBW)
The angle between the points where gain drops by 3 dB from its peak value.
Main Lobe
The region of strongest radiation in the antenna pattern.
Sidelobes
Smaller radiation lobes outside the main beam.
Back Lobe
Radiation directed behind the main reflector, opposite the main beam.
Radiation Pattern
A graphical representation of how RF energy is distributed in space.
Pattern Symmetry
The degree to which the radiation pattern remains balanced across different planes.
Geometry and Alignment Terms
Focal Point
The location where reflected RF energy converges in a reflector antenna system.
Focal Length
The distance between the reflector and the focal region.
F/D Ratio
The ratio of focal length to reflector diameter. This affects feed design, illumination, and overall system geometry.
Antenna Alignment
The process of orienting the antenna toward the intended signal source or target.
Pointing Accuracy
The precision with which the antenna can be directed.
Pointing Loss
Performance degradation caused by misalignment between the antenna beam and the desired target.
Efficiency and Aperture Terms
Antenna Efficiency
The percentage of input RF power that is effectively radiated or received by the antenna.
Aperture Efficiency
The ratio of effective aperture to physical reflector area.
Effective Aperture
The area over which the antenna effectively collects usable RF energy.
Surface Loss
Loss caused by reflector surface imperfections or conductive limitations.
Ohmic Loss
Signal loss caused by electrical resistance in conductive materials.
Illumination Efficiency
A measure of how effectively feed energy is distributed across the reflector aperture.
Blockage Loss
Losses caused by the physical obstruction of the aperture by the feed, sub-reflector, or support structure.
RF Measurement and Testing Terms
Antenna Measurement Range
A facility used to evaluate antenna gain, beamwidth, polarization, pattern shape, and sidelobes.
Near-Field Region
The region close to the antenna where the electromagnetic field structure is complex and not yet fully formed.
Far-Field Region
The region where the radiation pattern stabilizes and electromagnetic waves behave as plane waves.
Compact Antenna Test Range (CATR)
A system that simulates far-field conditions within a confined indoor test space.
Antenna Calibration
The process of verifying antenna performance using known standards or reference measurements.
Reference Antenna
A calibrated antenna used as a measurement baseline.
RF Frequency and Signal Terms
Radio Frequency (RF)
Electromagnetic frequencies used for communications, radar, sensing, and test systems.
Microwave Frequencies
Typically frequencies from 1 GHz to 30 GHz.
Millimeter-Wave (mmWave)
Typically frequencies from 30 GHz to 300 GHz.
Wavelength
The physical distance between repeating peaks of an electromagnetic wave.
Frequency
The number of cycles per second of an electromagnetic wave.
Application Terms
Satellite Communications (SatCom)
Communication systems that use satellites to relay RF signals between locations.
Ground Station Antenna
A high-gain antenna used to communicate with orbiting satellites.
Uplink
Transmission from Earth to a satellite.
Downlink
Transmission from a satellite to Earth.
Radar Antenna
An antenna used to transmit signals and receive reflections for detection, tracking, and measurement.
Radar Cross Section (RCS)
A measure of how detectable an object is by radar.
Tracking Antenna
An antenna system capable of continuously pointing toward a moving satellite, aircraft, or target.
Telemetry
The transmission of measurement or status data from a remote system to a receiving station.
Common Frequency Bands
- L-Band: 1–2 GHz
- S-Band: 2–4 GHz
- C-Band: 4–8 GHz
- X-Band: 8–12 GHz
- Ku-Band: 12–18 GHz
- Ka-Band: 26–40 GHz
- Q-Band: 33–50 GHz
- V-Band: 50–75 GHz
- W-Band: 75–110 GHz
These frequency bands are widely used in satellite communications, radar systems, wireless links, and millimeter-wave research applications.
Interested in this product or other Mi-Wave solutions?
Contact our team to discuss your frequency range, interface needs, and application requirements.
Custom configurations are available for specialized RF, microwave, and millimeter-wave systems.
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