风力涡轮机和射电天文服务的兼容性

IF 1.5 Q3 ASTRONOMY & ASTROPHYSICS Journal of Astronomical Instrumentation Pub Date : 2018-12-11 DOI:10.1142/S2251171719400026
B. Winkel, A. Jessner
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引用次数: 1

摘要

现代无线电天文设施不仅能够探测到来自宇宙的极弱电磁信号,还能够探测到各种来源的人造射频干扰。这些范围从想要的信号到无线电服务和应用的不想要的带外发射,再到各种电子和电气设备产生的电磁干扰。能量收集风力涡轮机不仅配备了电力转换硬件,还配备了大量的电子设备来控制和监测涡轮机。因此,射电望远镜附近的风力涡轮机可能会导致有害干扰,破坏测量的天文数据。许多天文台寻求与风力涡轮机制造商和运营商以及当地规划部门协调新风电场的布局,以避免出现这种情况。在我们的研究中,我们提供了确定风力涡轮机和无线电天文台之间间隔距离的示例和指南,以实现两者的良性共存。拟议的计算需要三个基本步骤。首先,根据适用于工业设备的欧洲EN 550011(CISPR,2015)标准,确定了预期的最大发射功率水平。其次,通过国际电信联盟提供的模型计算到达无线电接收器的路径上的传播损耗。最后,将接收功率与所考虑的受保护无线电天文观测频带中的允许功率限制进行比较。可以对望远镜站点周围的每个位置执行该程序,以便获得潜在有问题的风力涡轮机位置的地图。
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Compatibility Between Wind Turbines and the Radio Astronomy Service
Modern radio astronomical facilities are able to detect extremely weak electromagnetic signals not only from the universe but also from man-made radio frequency interference of various origins. These range from wanted signals to unwanted out-of-band emission of radio services and applications to electromagnetic interference produced by all kinds of electronic and electric devices. Energy harvesting wind turbines are not only equipped with electric power conversion hardware but also copious amounts of electronics to control and monitor the turbines. A wind turbine in the vicinity of a radio telescope could therefore lead to harmful interference, corrupting the measured astronomical data. Many observatories seek to coordinate placement of new wind farms with wind turbine manufacturers and operators, as well as with the local planning authorities, to avoid such a situation. In our study, we provide examples as well as guidelines for the determination of the separation distances between wind turbines and radio observatories, to enable a benign co-existence for both. The proposed calculations entail three basic steps. At first, the anticipated maximum emitted power level based on the European EN 550011 ( CISPR, 2015 ) standard, which applies to industrial devices, is determined. Then secondly, the propagation loss along the path to the radio receiver is computed via a model provided by the international telecommunication union. Finally, the received power is compared to the permitted power limit that pertains in the protected radio astronomical observing band under consideration. This procedure may be carried out for each location around a telescope site, in order to obtain a map of potentially problematic wind turbine positions.
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来源期刊
Journal of Astronomical Instrumentation
Journal of Astronomical Instrumentation ASTRONOMY & ASTROPHYSICS-
CiteScore
2.30
自引率
7.70%
发文量
19
期刊介绍: The Journal of Astronomical Instrumentation (JAI) publishes papers describing instruments and components being proposed, developed, under construction and in use. JAI also publishes papers that describe facility operations, lessons learned in design, construction, and operation, algorithms and their implementations, and techniques, including calibration, that are fundamental elements of instrumentation. The journal focuses on astronomical instrumentation topics in all wavebands (Radio to Gamma-Ray) and includes the disciplines of Heliophysics, Space Weather, Lunar and Planetary Science, Exoplanet Exploration, and Astroparticle Observation (cosmic rays, cosmic neutrinos, etc.). Concepts, designs, components, algorithms, integrated systems, operations, data archiving techniques and lessons learned applicable but not limited to the following platforms are pertinent to this journal. Example topics are listed below each platform, and it is recognized that many of these topics are relevant to multiple platforms. Relevant platforms include: Ground-based observatories[...] Stratospheric aircraft[...] Balloons and suborbital rockets[...] Space-based observatories and systems[...] Landers and rovers, and other planetary-based instrument concepts[...]
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