Research Article  Open Access
Guolong He, Xin Gao, Hui Zhou, "Fast Phased Array Calibration by PowerOnly Measurements Twice for Each Antenna Element", International Journal of Antennas and Propagation, vol. 2019, Article ID 6432149, 10 pages, 2019. https://doi.org/10.1155/2019/6432149
Fast Phased Array Calibration by PowerOnly Measurements Twice for Each Antenna Element
Abstract
This paper proposes a novel poweronly measurement method for phased array antenna calibration. Besides the total array power, only one phase shift and two power measurements for each array element are required to determine the element complex electric field distortion, one by shifting the element’s phase of and the other by turning the element under test off. The theory of the proposed calibration method is given, and the closed form formulation of the element amplitude and phase distortions is derived. From the mathematical point of view, it is the minimum required measurements that use two scalar values to determine one complex vector. Numerical simulations and experiments are conducted to validate and demonstrate the effectiveness of the proposed calibration method.
1. Introduction
Phased array antenna plays a very important role in modern radar and wireless communication systems [1–9]. Due to some inevitable errors and uncertainties, such as mechanical manufacturing tolerance, temperature variation, and electronic and radiofrequency component aging, the realistic array element excitation (both amplitude and phase) deviates from their ideal values. This would cause array radiation pattern distortion and degrade the overall performance, which must be carefully considered for practical system design. Hence, to maintain an acceptable performance of phased array antenna, calibrations are always necessary by measuring the excitation distortions of individual array elements and compensating them as accurate as possible before and/or during their operation.
A variety of calibration techniques have been proposed so far for phased array antenna calibration [10–23]. In [10], Silverstein proposed a method which controls the element phases based on timemultiplexed orthogonal codes; thus, the individual element excitation can be derived from the combined array signal. Some other phase toggling methods change the element’s phase shift to gather the required element excitation information [11–14]. Lee et al. [11] switched the element’s phase between the two states of 0 and and determined the element excitation by comparing the combined array signal at these two states. For all the abovementioned methods, they require coherent measurement between the calibration source and sink to obtain the complex value containing both amplitude and phase information. It is not always convenient to apply them for operating phased array system, especially for farfield calibration scenario with a long distance between the source and sink or in the millimeter wave band where the phase is sensitive and can be measured only with a restricted accuracy.
Compared to these complex measurement methods, some other methods which involve amplitude (or power) only measurements are considered to be more robust and convenient. In such case, coherent measurements are no longer required with precise synchronization between the transmitter and receiver. Many efforts have also been made that follow this principle. He et al. [15] proposed a method by periodically modulating the element phase sequentially and then applying a fast Fourier transform (FFT) analysis; the element complex electric field excitation is obtained from the corresponding modulation frequency harmonics of the combined array signal. The rotating element electric field vector (REV) method is another wellknown poweronly measurement method; it measures the amplitude of the array by shifting the element phase from 0 to 2 continuously [16, 17]. The element complex electric field can be determined from statistical signal processing of the three parameters, the maximum and minimum power of the array signal, and the element rotation phase to maximum power. Although it is very simple and easy to use, however, a large amount of measurements for each element is needed in the conventional REV method. In 2001, Sorace [18] pointed out that measurement results at four orthogonal phase shifts are sufficient enough to obtain a maximum likelihood estimation for each array element. Long et al. [19] also derived an expression that requires two phase shifts of and to yield the element complex excitation information. All these above efforts are made to reduce the amount of required measurements and overcome the inefficiency of the original REV method.
In this paper, we propose a novel poweronly measurement method to calibrate the element complex excitation distortion. For each array element, two power measurements are enough to determine the element complex electric field, one by shifting the element’s phase of and the other by turning the element under test off. This method only needs some simple mathematical calculation but requires no auxiliary calibration element or any additional hardware. From the mathematical point of view, it is the minimum required measurements that use two scalar values to determine one complex vector. The rest of this paper is organized as follows. In Section 2, the proposed calibration method is introduced, and the closedform formulation for element amplitude and phase distortions is derived. Then, in Section 3, the calibration accuracy is analyzed mathematically; the standard derivations of both the amplitude and phase estimations are obtained. Section 4 uses an eightelement patch antenna array to demonstrate the calibration procedure and investigate its performance. In Section 4, a fourelement dipole antenna array is fabricated and tested to further validate the effectiveness of the proposed method. Finally, this paper is concluded in Section 5.
2. Methodology
Figure 1 illustrates a typical configuration for element active phased antenna array. It contains both transmitting and receiving modes by adopting the T/R module. Each antenna element has a phase shift for electronic beam scanning. The method proposed in this paper can be used in not only the transmitting mode but also the receiving mode. Let and denote the amplitude and phase of the th antenna element, . The phased array electric field , the combination of the individual element electric fields, can be described as follows: where and are the amplitude and phase of the array electric field, respectively. As shown in Figure 2, in order to calibrate the th array element complex excitation distortion, we can divide equation (1) into two parts: where denotes the combined electric field of the array expecting the th element, and it has the power of which can be easily measured by turning the th element under test off or terminating it with a matched load.
From equation (2), the array power can be expressed as
We denote the phase difference ; thus, equation (3) can be further rewritten as where and are the real and imaginary parts of the th array element complex excitation, respectively.
We then shift the phase of the th antenna element by ; then, the corresponding electric filed and the array power can be written as
From equations (4) and (6), the two unknowns and can be derived as follows: or where
Since is the same for all the elements, thus, only two additional poweronly measurements and are required to calculate each element excitation distortion. Like the conventional REV method, it also has two possible solutions in equations (7a) and (7b). This ambiguity can be easily eliminated if the initial phases of the individual elements are set to make [19]. From equations (7a) and (7b), the relative amplitude and phase distortion, and , of the th antenna element compared to the array signal can be derived as where
3. Calibration Accuracy Analysis
Recall that and are the real and imaginary parts of the th array element complex excitation, respectively. Since these two components are orthogonal to each other, they can be modeled as independent Gaussian distributions with zero mean and the variance , where SNR is the signaltonoise ratio of the power measurement. By squaring them and adding together as in equation (10a), the result of should have doubly noncentral chisquared distribution with two degrees of freedom. From the above derivation, the amplitude estimation , as the square root of , should have a Rayleigh distribution, and it has the standard deviation as [14]
The phase estimation , as shown in equation (10b), can be viewed as the ratio of two Gaussian distributions. Its probability density function (PDF) can be expressed as follows [24]: where also has approximate Gaussian distribution for high SNR. Finally, the standard deviation of the phase estimation in degree is approximated as [14]
4. Numerical Simulations
In order to verify the effectiveness of the proposed method, an eightelement linear patch antenna array working at Sband is numerically simulated to demonstrate the calibration procedure and evaluate its performance. The phased array contains eight halfwavelength spaced patch antenna elements. As shown in Figure 3, the rectangular patch antennas are with length cm and width cm on the lossless substrate, which has the dielectric constant and thickness of 1.57 mm. The feed is offset by 5.5 mm from the center of the rectangular patch antenna.
During the simulation, random initial amplitude and phase excitation are preset for each antenna element. The standard deviation for element amplitude and phase error is set to 0.5 dB and 10 deg, respectively. The power measurement is made at the farfield region of the phased array, and the measurement SNR is set as 20 dB. Figure 4 illustrates one example of the simulated farfield power measurement results. The black asterisks denote the normalized combined array power P_{0}, which is normalized to 0 dB. The red and blue triangles denote the two power measurements and for each array element. They vary from each other since every element has different amplitudes and phase distortions. Figures 5 and 6 illustrate the calibration results for each element derived from the proposed method. Compared to the preset values, the corresponding calibration errors are 0.26 dB and 2.17 deg for amplitude and phase distortion, respectively. It can be seen that the estimation results have very good coincidence with the preset values. The investigation is further conducted by 1000 Monte Carlo simulations. The histogram of element amplitude and phase calibration errors is presented in Figures 7 and 8, both of which show nearly normal distributions. Moreover, approximately 84% of the amplitude calibration errors fall in the region of 1 dB and +1 dB, while the probability percentage of phase calibration error in the range of 5 deg to +5 deg is nearly 78%. The standard deviations of element amplitude and phase estimation errors for different SNR conditions are presented in Figures 9 and 10. It can be seen from the results that the mean square error (MSE) of both amplitude and phase calibration decreases dramatically with the increase of the SNR. For SNR larger than 30 dB (this condition can be easily achieved in practice), the amplitude and phased calibration error are less than 0.05 dB and 0.5 deg; such high accuracy exceeds most phased array calibration demands.
5. Experiment Demonstration
To further validate the effectiveness of the proposed method, a fourelement dipole antenna phased array is fabricated and tested. As shown in Figure 11, this antenna array works at Sband with full transmitting and receiving duplex function. For the transmitting mode calibration, a pure sinusoidal wave source is fed to the phased antenna array, the signal goes to each antenna element from the digital beamforming network (DBF) then transmits to the free space, and a calibration receiver is placed at the far field of the phased array and connected with a power meter or spectrum analyzer, while for the receiving mode calibration, the calibration transmitter at the farfield region transmits a pure sinusoidal wave, and the phased array receives the plane wave by the elements and the combined array signal is connected to a power meter.
The phased array calibration process is described as follows: (1)First, each antenna element is measured individually using a vertical network analyzer (VNA), and their amplitude and phase distortions are obtained(2)The combined power of the test array is measured by a power meter(3)By setting the DBF weight of the th antenna element to zero sequentially, the combined power of the array expecting the th element is measured by a power meter(4)By setting the phase of the th antenna element to sequentially, the combined power of the array is measured by a power meter(5)The amplitude and phase calibration results are calculated by using equation (9) and compared with the results from step (1)
Both the transmitting and receiving modes are carefully calibrated in our work. The results of the receiving mode are presented in Table 1, while the results of the transmitting mode are similar and are not given here for the constraint of the paper length. During the experiments, the power measurements are accomplished by using Agilent E4405B Spectrum Analyzer, while Keysight M9374A PXIe Vector Network Analyzer is used for singleantenna element calibration. The reading accuracy of the power and phase measurements is set as 0.1 dB and 0.1 deg, respectively. Figures 12 and 13 illustrate the calibration results by our method with the results from VNA measurement. The results by using Long et al.’s method in [19] are also presented for comparison. It can be seen that both the amplitude and phase calibration results by our method have good agreement with the measurement results from VNA and the results from Long et al.’s method. The corresponding standard deviations are 0.06 dB for amplitude calibration and 0.37 deg for phase calibration.

6. Conclusion
Phased array element excitation (both amplitude and phase) always deviates from the ideal values that would cause array performance degradation, which must be carefully calibrated and compensated as accurate as possible for practical phased array system design. This paper proposes a novel power measurement method to obtain the excitation distortions of individual array elements. Besides the total array power, only one phase shift and two power measurements for each array element are required to determine the element complex excitation, one by shifting the element’s phase of and the other by turning the element under test off. This method only involves some simple mathematical calculation and requires no auxiliary calibration element or any additional hardware. From the mathematical point of view, it is the minimum required measurements that use two scalar values to determine one complex vector. An eightelement linear patch antenna array is numerically simulated to demonstrate the calibration procedure, and the calibration performance is investigated by Monte Carlo simulations. Furthermore, a fourelement dipole antenna array is fabricated and tested to validate the effectiveness of the proposed method.
Data Availability
The data used to support the findings of this study are available from the corresponding author on reasonable request.
Conflicts of Interest
The authors declare that there are no conflicts of interest regarding the publication of this paper.
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Copyright
Copyright © 2019 Guolong He et al. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.