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Considering the width of main lobe provided in Figure7, for the case of 33 Hz distance, the second lobes of two AF estimations would overlap together.
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Therefore, the directional antenna can provide the same EIRP in the main lobe direction as that an omnidirectional antenna provides while using much less transmit power than that the omni-direction antennas uses.
It is clear that the DA [35] and GSMDS models provide the similar main lobe width, and both of them outperform the conventional beamforming (CBF, i.e., DAS beamforming) model.
The simplest approach is the beamforming that provides noise source maps with large main lobe and strong side lobes at low frequency.
The proposed filter provides wideband compensation over the specified CIC main lobe bandwidth.
Choosing allows multiple side lobes of the sinc function to alias in on the main lobe.
With synthetic data, we show that the side lobes are removed and the main lobe is narrower.
Usually, in photographic images of stars, the side lobes do not show up, but you do see the width of the main lobe.
For the larger soliton order case, the spectral main lobe may vary its position.
Five chirp schemes were designed to investigate the relationship of the range side lobe level (RSLL), main lobe width and energy for strain imaging.
Moreover, unlike conventional transducers, the pencil beam can be effectively steered over a wide range of angles without producing grating lobes or degrading the power difference between the main lobe and side lobes.
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