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Offset spherical reflector antenna with low cross-polarisation

机译:偏移球形反射器天线,交叉极化低

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In view of the emphasis now attached to low sidelobe envelopes for satellite communications, an increasing importance has been given to dual offset antennas for small Earth stations. The above mentioned offset geometry is particularly interesting because it avoids subreflector and feed blockages which are responsible for rising sidelobes. The spillover effects in the offset plane can be minimised by aligning the plane of offset orthogonally to the geostationary orbit. Attracted by the costs characteristics of the spherical reflector, the authors present a few modifications in the geometry initially considered by P. Ramanujan et al. (see IEE Proc. H, vol.134, no.2, p.199-204 (1987)). These modifications lead to designs with a higher efficiency, a larger clearance from the sidelobe specifications, and a significant reduction on the farfield cross-polarisation. To illustrate this the authors use the Gregorian configuration.
机译:鉴于现在附加到卫星通信的低侧瓣信封的重点,对小地球站的双偏移天线提供了越来越重要的重要性。 上面提到的偏移几何形状特别有趣,因为它避免了负责上升侧瓣的子折叠器和馈送堵塞。 通过使偏移平面与地球静止轨道对齐,可以最小化偏移平面中的溢出效应。 由球面反射器的成本特性引起,作者在最初由P. Ramanujan等人考虑的几何图中存在一些修改。 (见IEE Proc。H,Vol.134,No.2,P.199-204(1987))。 这些修改导致效率更高的设计,从侧链规格的间隙较大,以及对法交叉极化的显着降低。 为了说明这,作者使用Gregorian配置。

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