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Microwave Engineering Europe Magazine

The 2000 CAD Benchmark Unveiled

Over the past few years the series of CAD Benchmarks in Microwave Engineering Europe has proved an enduring favourite among our readers, none more so than those challenging the capabilities of 3D electromagnetic simulators. This year for the first time we have chosen to benchmark the performance of these packages in simulating a free space radiation problem - a balanced antipodal Vivaldi antenna - whose characteristics are described below. This problem has been circulated to a broad group of CAD vendors, and we will publish their solutions in the November issue. Readers are invited to attempt their own solutions to the Benchmark, and can post solutions, comments or questions to the vendors on our Web site at www.mwee.com.

Send us your comments on this article

Download the article in Adobe PDF format [approx 175 kB]

    Figure 1. 3D representation of balanced Vivaldi antenna. Yellow is stripline track/flare, brown is lower groundplane transition/flare, and purple (unshaded) is upper ground plane transition/flare, which is the same as the lower groundplane. Cyan is the substrate outline.


The conventional Vivaldi antenna typically has at least an octave bandwidth making it suitable for a wide variety of applications, but can be limited by its radiating slot transition. The antipodal Vivaldi, in which a microstrip line and its groundplane both gradually flare out, removes the bandwidth limitations of the transition. The lower frequency limit is now determined by the cut-off mechanism of the flare, namely that the aperture is half a wave-length wide. However the skew in the electric fields across the slot leads to poor cross-polar performance, which also degrades as the frequency rises.

A development of the antipodal Vivaldi which remedies its worst characteristics is the subject of this Benchmark. Converting it to a triplate based structure, by adding in an additional dielectric and metallization layer which balances the E-field distribution in the flared slot, greatly improves its cross-polar performance.

The antenna starts in stripline. One side of a board has the input track which is then flared to produce one half of a conventional Vivaldi. On the other side (and on the second substrate) the ground planes are reduced down to form what will be a balanced set of lines. The 'ground lines' are then flared out in the opposite direction to form the overall balanced antipodal Vivaldi.

The configuration uses arcs and elliptically tapered geometry which can be a good test for some solver software and, along with the aim of predicting certain far-field characteristics, led us to conclude that this would be a non-trivial but feasible benchmark. Another interesting aspect will be to see how the Vendors determine their air-boxes, radiation boundaries etc, unlike a closed waveguide or stripline problem. This is usually an arbitrary aspect in most software and a source of uncertainty and error for inexperienced users.

Dimensional data

Figures 2 to 5 give most of the dimensional detail. The key points are as follows:-

  • Substrate is 40mm wide. A length of 90mm is adequate for defining all the detail
  • Stripline track width is 3mm
  • Output flares are elliptical arcs 30mm long by 9mm high, representing a 3.33:1 major/minor axis ratio
  • Transitions from groundplane to balanced line are also elliptical
  • Aperture slot width is 15mm
  • Port/edge info: apart from the input edge, all other edges are exposed dielectric. At the input edge metal is present connecting the two ground planes together except for a 12mm wide area centred around the track where the excitation port is present (a SMA edge launcher in practice). See Figure 4 for this detail.

    Figure 2. General geometry and aperture detail.

    Figure 3. Central (stripline) metallization layer. Note: Output flare and radius also to the groundplane layers.

    Substrate

    The substrate used in this example is Rogers Duroid 5870: r =2.32, width 40mm, length 90mm. Two 1.575mm (0.062") thick boards are used to create the overall triplate structure. Metallization thickness and loss tangents may be ignored if necessary. Other than the edges near the port mentioned above, no other edge metallization or vias are present. Examples of these antennas have been fabricated on higher r substrates as well, particularly in array applications.

    Figure 4. Outer ground plane layers. Note: There is a short straight section between the end of the transition and the start of the aperture flares.

    Figure 5. Perspective view and input port edge detail. Note: Stripline track layer is sandwiched by two 1.575mm thick duroid layers.

     

    Outputs

    A reasonable amount of background information is requested to make the assessment more informed, as well as the analysis results themselves. The following outputs are expected from the CAD vendors:-

  • Model geometry printout with annotation which would confirm dimensions/ approximations used, boundary regions/definitions (e.g. air volumes, excitations, radiation boundaries etc), as well as feedback on ease of definition etc.
  • S-Parameters and input impedance: A minimum analysis range of 0.5 -10GHz is required, but optionally higher (the original device was characterised up to 18/20 GHz). Plots (in dB vs. frequency format), and Touchstone format files for return loss are needed (to make replotting and comparisons easier)
  • Pattern data output at 10.0GHz for E- and H-plane cuts, co- and cross-polar, gain, beamwidth. plots should be in Cartesian format in dB vs. degrees. Optionally 3D colourful plots/animations may be submitted electronically to illustrate features. As this is principally an antenna benchmark, emphasis will be on these results.
  • Comments on problem entry/setup, solution process etc, discussion of results
  • Hardware data: make/model, operating system, clock speed, RAM fitted, number of CPUs
  • Software data: name, version, elapsed run times, RAM/disk space needed, number of elements used (or cells/ unknowns)

     

    The first part of this Focus can be viewed here .

    Microwave Engineering welcomes your comments about this article.

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    E-mail:

    Your comments:

     

     

    « October Issue








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