Equation Section 1
METHODS TO ESTIMATE AND REDUCE LEAKAGE BIAS ERRORS IN PLANAR NEAR-FIELD ANTENNA MEASUREMENTS
Allen C. Newell Newell Near-Field Consultants
2305 Vassar Drive, Boulder CO 80305
Jeff Guerrieri and Katie MacReynolds
National Institute of Standards and Technology
325 Broadway, Boulder, CO 80305
This paper describes two methods that can be used to measure the leakage signals in quadrature detectors, predict the effect on the far-field pattern, and correct the measured data for leakage bias errors without additional near-field measurements. One method is an extension and addition to the work previously reported by Rousseau1. An alternative method will be discussed to determine the leakage signal by summing the near-field data at the edges of the scan rather than summing below a threshold level. Examples for both broad-beam horns and narrow-beam antennas will be used to illustrate the techniques.
Antenna measurements; Error correction; Planar near-field; Quadrature detector
U.S. Government contribution not subject to copyright in the United States.
The leakage arising from the receiver bias error cannot generally be reduced with user-available changes in instrumentation. The error arises from very low-level residual offset errors in the wideband quadrature detectors that produce voltages proportional to the real and imaginary parts of the measured signals. The level of the leakage signal also may depend on the measurement frequency and the particular hardware configuration and needs to be checked for each measurement. This type of bias leakage signal is found on all microwave receivers that use quadrature detection for measuring amplitude and phase.
Terminating the transmission lines connected to the AUT or the probe and making a near-field measurement allows measurement of the leakage signal. The measured signal will be a combination of the noise level of the receiver and the leakage signal.
Figure 1. Sample of NF data, leakage data and calculate leakage from average of measurement.
A principle plane cut for one such measurement is shown in Figure 1 along with the same cut for the AUT, a standard gain horn (SGH). Depending on the receiver averaging and the random error, the bias leakage signal may be equal to or lower than the measured near-field amplitude. It can be found by calculating the sum of the real and imaginary parts of the measured data. The magnitude of the resulting sum is equal to the bias-signal level and is shown as the third curve in Figure 1. Another example is shown in Figure 2, where a receiver averaging of 26 msec was used, compared to 0.3 msec for the data of Figure 1. In this case the calculated average is essentially equal to the measured leakage signal.
Figure 2. Sample of NF data, leakage data and calculate leakage from average of measurement.
Of more importance than the near-field leakage level is quantifying the effect of the bias leakage on the far-field pattern. This effect will depend on the AUT properties as well as the near-field measurement parameters. As illustrated in Figure 3, the constant amplitude and phase of the bias leakage signal transforms to a narrow beam pattern centered along the Z-axis direction. It will therefore have the major effect on the on-axis gain and the on-axis cross- polarized
Figure 3. AUT FF pattern and bias leakage far-field for the data in Figure 2.
(1) d ís are the data-point spacings in x and y, denotes the measured data, are the transverse part of the propagation and position vectors respectively. Noting that the far-field peak is the product of the near-field voltage times an area; we can approximate the far-field peak from the equation
»10 log ( N
AUT Ae )
N AUT = Near-field Peak Amplitude,(2)
Ae = Near-field Effective Area of AUT. For a typical antenna, the near-field effective area will be less than the actual physical area of the antenna and approximately equal to the conventional effective area. If the leakage signal has a constant amplitude and phase independent of the probe position, as produced by the receiver bias error, the near-field effective area is the full scan area. If the leakage varies in amplitude and phase as a function of position, as caused by cable leakage, the near-field effective area will be less than the full measurement area. There fore, from Equation (2). (3) The AUT near-field effective area can be estimated from the physical area of the antenna or calculated from the far-field peak and Equation (2) after completing the near-field measurements. Then from the observed leakage near-field amplitude and Equation (3) we can determine the leakage far-field peak relative to the main and cross component patterns. The third term in Equation (3) referred to as the leakage gain defines the increase in relative amplitude between the leakage signal and the AUT signal between measured near-field and calculated far field. Note that this term is proportional to the square of the effective areas and not measurement areas. For typical measurements, the measurement area is much larger than the AUT to reduce errors due to truncation and to maximize the angular coverage. This can result in a leakage gain on the order of 25 to 50 dB and illustrates why it is important to measure the bias leakage level and correct for it where possible. The correction is performed on the measured data using a script that subtracts a constant amplitude and phase signal from the measured data. If the leakage signal has been correctly measured, the result is a data set that should show little if any effect on the far-field pattern. Figures 4 and 5 show examples of two cases where the leakage signal has the large effect. Figure 4 shows the main component peak for a broad beam antenna such as a standard gain horn typically used as a gain reference. Figure 5 shows an example of the cross-polarized pattern characteristic of many antennas.
Figure 4. Illustration of leakage correction on the main component of a horn antenna. In the first case, the effective area of the horn is relatively small and measurements are generally made over a large area to reduce the effect of truncation. As a result the leakage gain in Equation (3) is on the order of 40 dB. The leakage error can cause uncertainties on the order of 0.1 dB in the far-field pattern for the horn measurement, which is significant for a gain-standard antenna.
Figure 5. Illustration of leakage correction on the cross component far-field pattern. In the second case, the far-field amplitude for the cross-polarized pattern is generally 30 to 50 dB below the main-component. With leakage gains of 30 to 50 dB the far-field leakage becomes comparable to the cross component, resulting in the null on-axis shown in Figure 5.
Since the cross-polarized pattern may often have an on-axis null like this, it is difficult to tell whether it is due to leakage without performing the correction.
Figure 6. Example of threshold calculation method for determining bias leakage level.
As a result, an alternative method has been developed that
calculates the leakage level by determining the change in the on-axis value
of the main and cross components when a given number of rows and columns
of data are truncated from the near-field data. On close inspection, it
was found that the end result of this calculation was the same as Equation
(4) except that the sum is performed over the truncated data rather than
over the data below a certain threshold.
(6)are the indices within the truncated region. The calculation can be carried out efficiently using the truncation feature built into the software. When this calculation is used on the same near-field data used in Figure 6, the result for the amplitude is shown in Figure 7. The truncation covered approximately the same region of the measured data as the threshold method. In general, the two methods usually gave very similar results, but in some cases, the truncation method was easier to interpret since the curve was flat over a larger region and did not require identifying a plateau region.
Figure 7. Example of truncation calculation method for determining bias leakage level.
It is not clear why the truncation method appears to work better in some cases. One possibility is illustrated in Figure 8, which shows a schematic comparison of the data that is summed in the two methods. The horizontal lines represent the "slices" of data that are summed in the threshold method. At the low levels, there may be very few points to sum and the threshold method does not sum all adjacent measured points. As a result, the sum may not converge to the constant-leakage level until the threshold is above the region where there are oscillations in the data. The "slices" of data that are summed in the truncation method are represented by the vertical lines. Adjacent points are always summed and the far-out points contribute very little to the main beam. The truncation sum will then converge sooner to the leakage level even in the region where there are oscillations in the data.
Figure 8. Near-field amplitude and summation regions for two methods.
Two methods have been demonstrated for measuring the bias leakage level and
predicting its effect on the far-field pattern. The first method uses a single
measurement with the receiver on high average and provides a direct measurement
of the leakage amplitude and phase. Equations can then be used to calculate
the effect on the far field, and the leakage can also be subtracted from the
measured data. In the second method, the bias leakage signal is determined by
summing the measured data using either the threshold or truncation method. Once
it has been measured, it can be subtracted from the measurement to reduce or
eliminate far-field errors.
1 Rousseau, P. R., "An algorithm to reduce errors in planar near-field measurement
data, AMTA Proceedings, Oct. 1999, pp 269-271.
1 Rousseau, P. R., "An algorithm to reduce errors in planar near-field measurement data, AMTA Proceedings, Oct. 1999, pp 269-271.