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Numerical model of the QiTai radio Telescope PAF receiver signal and simulation of interference mitigation
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Xinjiang Qitai is constructing a 110-m fully steerable radio telescope (QiTai radio Telescope [QTT]) equipped with a phased array feeds (PAF) receiver, which will install the focal plane operating from 0.7 to 1.8 GHz. In this article, we introduce a PAF receiver model for beamforming, and the numerical model of the internal and external noise for this PAF receiver is provided using electromagnetic field simulation software. The linear constraint minimum variance (LCMV) algorithm is used to simulate the interference mitigation. The interference mitigation rate is from 0.581 to 0.921, and the signal restoration rate is from 0.998 to 1.512 within the error range of an interference arrival angle of 10°. This conclusion can be used in the signal correction of the PAF receiver for interference mitigation.
Title: Numerical model of the QiTai radio Telescope PAF receiver signal and simulation of interference mitigation
Description:
Xinjiang Qitai is constructing a 110-m fully steerable radio telescope (QiTai radio Telescope [QTT]) equipped with a phased array feeds (PAF) receiver, which will install the focal plane operating from 0.
7 to 1.
8 GHz.
In this article, we introduce a PAF receiver model for beamforming, and the numerical model of the internal and external noise for this PAF receiver is provided using electromagnetic field simulation software.
The linear constraint minimum variance (LCMV) algorithm is used to simulate the interference mitigation.
The interference mitigation rate is from 0.
581 to 0.
921, and the signal restoration rate is from 0.
998 to 1.
512 within the error range of an interference arrival angle of 10°.
This conclusion can be used in the signal correction of the PAF receiver for interference mitigation.
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