PopHorn: A deployable folding horn antenna for low frequency space-based applications

PopHorn:适用于低频天基应用的可展开折叠喇叭天线

基本信息

  • 批准号:
    ST/Y509942/1
  • 负责人:
  • 金额:
    $ 64.02万
  • 依托单位:
  • 依托单位国家:
    英国
  • 项目类别:
    Research Grant
  • 财政年份:
    2024
  • 资助国家:
    英国
  • 起止时间:
    2024 至 无数据
  • 项目状态:
    未结题

项目摘要

Different shapes and types of radio antennas are useful in different circumstances. Horn-shaped antennas are particularly good for when a very accurate calibration of some radio instrumentation (e.g. a radio telescope) is needed, for example. This makes horn antennas very popular for many different applications at microwave frequencies, where they only need to be a few centimetres (or tens of centimetres) across. At low frequencies, a horn antenna would have to be gigantic to work in the same way however. This large size limits their usefulness, particularly for space-based applications where there are restrictive requirements on size and weight of the payloads. We will develop a type of folding antenna that can be packaged up into a relatively small and lightweight form suitable for attaching to a spacecraft, but which folds out into a large horn antenna shape when deployed, suitable for low-frequency applications. This will make it practical to do very high precision radio measurements at low frequencies from space.
不同形状和类型的无线电天线适用于不同的情况。例如,当需要对某些无线电仪器(例如射电望远镜)进行非常精确的校准时,喇叭形天线特别有用。这使得喇叭天线在微波频率的许多不同应用中非常受欢迎,它们的宽度只需几厘米(或几十厘米)。然而,在低频下,喇叭天线必须很大才能以同样的方式工作。这种大尺寸限制了它们的实用性,特别是对于有效载荷的尺寸和重量有限制性要求的太空应用。我们将开发一种折叠天线,它可以封装成相对较小且重量轻的形式,适合连接到航天器上,但在部署时折叠成大喇叭天线形状,适合低频应用。这将使在太空低频下进行高精度无线电测量成为现实。

项目成果

期刊论文数量(0)
专著数量(0)
科研奖励数量(0)
会议论文数量(0)
专利数量(0)

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Philip Bull其他文献

Constraining Post-Newtonian Parameters with the Cosmic Microwave Background
用宇宙微波背景约束后牛顿参数
  • DOI:
  • 发表时间:
    2024
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Daniel B. Thomas;Theodore Anton;Timothy Clifton;Philip Bull
  • 通讯作者:
    Philip Bull
Direct Optimal Mapping Image Power Spectrum and its Window Functions
直接最优映射图像功率谱及其窗函数
  • DOI:
  • 发表时间:
    2023
  • 期刊:
  • 影响因子:
    0
  • 作者:
    Zhilei Xu;Honggeun Kim;J. Hewitt;Kai;N. Kern;Elizabeth Rath;R. Byrne;Adélie Gorce;Z. Martinot;J. Dillon;B. Hazelton;Adrian Liu;M. Morales;Z. Abdurashidova;Tyrone Adams;J. Aguirre;Paul Alexander;Z. Ali;R. Baartman;Yanga Balfour;A. Beardsley;G. Bernardi;T. Billings;J. Bowman;R. Bradley;Philip Bull;J. Burba;S. Carey;C. Carilli;Carina Cheng;D. DeBoer;E. D. L. Acedo;M. Dexter;N. Eksteen;J. Ely;A. Ewall;N. Fagnoni;R. Fritz;S. Furlanetto;K. Gale;B. Glendenning;D. Gorthi;B. Greig;J. Grobbelaar;Z. Halday;J. Hickish;D. Jacobs;A. Julius;M. Kariseb;J. Kerrigan;P. Kittiwisit;S. Kohn;M. Kolopanis;A. Lanman;P. Plante;A. Loots;D. MacMahon;L. Malan;C. Malgas;K. Malgas;B. Marero;A. Mesinger;M. Molewa;Tshegofalang Mosiane;S. Murray;A. Neben;B. Nikolic;H. Nuwegeld;A. Parsons;Nipanjana Patra;Samantha Pieterse;N. Razavi;J. Robnett;K. Rosie;P. Sims;Craig H. Smith;H. Swarts;N. Thyagarajan;P. V. Wyngaarden;P. Williams;Haoxuan Zheng
  • 通讯作者:
    Haoxuan Zheng

Philip Bull的其他文献

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{{ truncateString('Philip Bull', 18)}}的其他基金

Pushing 21cm to the (statistical) limit: A first EoR detection with an SKA Precursor
将 21 厘米推向(统计)极限:使用 SKA Precursor 进行首次 EoR 检测
  • 批准号:
    ST/X002624/1
  • 财政年份:
    2022
  • 资助金额:
    $ 64.02万
  • 项目类别:
    Research Grant

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