Study of free-space coupling into mm-wave whispering-gallery mode resonators for a radioastronomy receiver

被引：0
|
作者：
Santamaria-Botello, Gabriel [1 ]
Atia Abdalmalak, Kerlos [1 ]
Schlecht, Maria-Theresa [2 ]
Gonzalez-Ovejero, David [3 ]
Sedlmeir, Florian [4 ]
Schwefel, Harald G. L. [4 ]
Malzer, Stefan [2 ]
Weber, Heiko [2 ]
Segovia-Vargas, Daniel [1 ]
McCarthy, Darragh [5 ]
Murphy, John Anthony [5 ]
Dohler, Gottfried H. [5 ]
Garcia Munoz, Luis Enrique [1 ]
机构：
[1] Univ Carlos III Madrid, Getafe, Spain
[2] Friedrich Alexander Erlangen Nurnberg Univ, Erlangen, Germany
[3] CALTECH, Pasadena, CA USA
[4] Univ Otago, Dunedin, New Zealand
[5] Maynooth Univ, Maynooth, Kildare, Ireland
来源：
2017 IEEE INTERNATIONAL SYMPOSIUM ON ANTENNAS AND PROPAGATION & USNC/URSI NATIONAL RADIO SCIENCE MEETING | 2017年
关键词：
D O I：
暂无
中图分类号：
TM [电工技术]; TN [电子技术、通信技术];
学科分类号：
0808 ; 0809 ;
摘要：
In this paper, the coupling mechanism of a free-space Gaussian beam into a whispering-gallery mode resonator through a dielectric lens is mathematically modeled and numerically solved by means of the Schelkunoff-Waterman method (the so called T-matrix method). This approach allows in principle, to quickly analyze the performance of different near-field coupling mechanisms with arbitrary excitations. The aim is to efficiently excite a WGM into a nonlinear dielectric resonator in order to detect the weak mm-wave radiation from the cosmic microwave background (CMB) by up-converting the signal into the optical domain via the nonlinearity of the medium.
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页码：1277 / 1278
页数：2
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