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Whiskers, hyperhemispheres, and a honeymoon

机译:晶须,半球和蜜月

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摘要

I plan to make a few historical comments on early research in antennas for submillimeter waves, as the area was known in the 1970's. The initial focus was on understanding the limits of the tungsten whiskers that were then used as antennas. However, as integrated-circuit technology improved, it became clear that planar antennas on semiconductor substrates were needed. However, these antennas interact strongly with substrate modes. One way to eliminate the substrate modes is to put a lens on the back of the substrate and to couple power in through the lens. These substrate-lens coupled antennas are widely used today in laboratory instruments and radio astronomy. Another approach to suppressing the substrate modes is through a periodic antenna structure. This is the basis for the grid amplifier, which combines the outputs of large numbers of transistors in free space. This allows much more transmitter power than was previously possible from solid-state devices. The Wavestream Corporation was founded to develop this technology. The company's best-selling product is a 50-W amplifier for 30-GHz satellite uplinks. Several thousand amplifiers have been sold to date.
机译:我计划就亚毫米波天线的早期研究做出一些历史性评论,因为该领域在1970年代就已广为人知。最初的重点是了解随后用作天线的钨晶须的极限。然而,随着集成电路技术的改进,很明显需要在半导体衬底上的平面天线。然而,这些天线与衬底模式强烈地相互作用。消除基板模式的一种方法是将透镜放在基板背面,并通过透镜耦合电源。这些衬底透镜耦合天线如今已广泛用于实验室仪器和射电天文学。抑制衬底模式的另一种方法是通过周期性天线结构。这是栅格放大器的基础,该栅格放大器在自由空间中合并了许多晶体管的输出。与固态设备以前相比,这可以提供更多的发射器功率。 Wavestream Corporation的成立是为了开发这项技术。该公司最畅销的产品是用于30 GHz卫星上行链路的50 W放大器。迄今为止,已经售出了数千台放大器。

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