Far-Sidelobe Antenna Pattern Measurement of LiteBIRD Low Frequency Telescope in 1/4 Scale
Far-Sidelobe Antenna Pattern Measurement of LiteBIRD Low Frequency Telescope in 1/4 Scale
复制标题
1/4 比例 LiteBIRD 低频望远镜远旁瓣天线方向图测量
DOI:
10.1109/tthz.2019.2937497
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发表时间:
2019
影响因子:
3.2
通讯作者:
Okada Norio
中科院分区:
文献类型:
--
作者:
Takakura Hayato;Sekimoto Yutaro;Inatani Junji;Kashima Shingo;Imada Hiroaki;Hasebe Takashi;Kaga Toru;Takeda Yoichi;Okada Norio
Polarization of the cosmic microwave background (CMB) has crucial information on the inflationary universe. To detect these signals, it is necessary to suppress far sidelobes of a telescope, which contaminate the CMB signals with strong foreground radiation, such as the Galactic plane. LiteBIRD is the only funded CMB observation satellite for the 2020s, and the low frequency telescope (LFT; 34-161 GHz) is one of its telescopes. We measured near-field antenna patterns of the LFT using its 1/4-scaled model and examined far sidelobes up to 60° from the peaks. To cover the 20° field of view of the LFT, we investigated the antenna patterns at the edges of the focal plane as well as at the center. The measurement frequencies were 140-220 GHz, which correspond to the lowest bands (35-55 GHz) of the full-scale LFT. The measurements were consistent with the simulated far-sidelobe patterns at least -50 dB level, and showed that far sidelobes for two orthogonal polarization directions are consistent with each other down to -40 dB level. We also measured the cross-polarization patterns, and their peak level was less than -20 dB.
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DOI:
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发表时间:
2009
期刊:
影响因子:
--
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10.1109/eumc.2008.4751564
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2008
期刊:
2008 38th European Microwave Conference
影响因子:
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2012
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DOI:
10.1117/12.2312185
发表时间:
2018
期刊:
Proc.SPIE Int.Soc.Opt.Eng.
影响因子:
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DOI:
10.1002/sat.4600110107
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1990
期刊:
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影响因子:
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作者:
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