Intertwined inductive frequency selective surface: An application for satellite communications

Vásquez Peralvo, Juan Andrés, Fernández González, José Manuel ORCID: https://orcid.org/0000-0002-9296-4098 and Rigelsford, Jonathan M. (2019). Intertwined inductive frequency selective surface: An application for satellite communications. En: "13th European Conference on Antennas and Propagation (EuCAP 2019)", 31/03/2019 - 05/04/2019, Cracovia, Polonia. ISBN 9781538681275. pp. 1-4.

Descripción

Título: Intertwined inductive frequency selective surface: An application for satellite communications
Autor/es:
  • Vásquez Peralvo, Juan Andrés
  • Fernández González, José Manuel https://orcid.org/0000-0002-9296-4098
  • Rigelsford, Jonathan M.
Tipo de Documento: Ponencia en Congreso o Jornada (Artículo)
Título del Evento: 13th European Conference on Antennas and Propagation (EuCAP 2019)
Fechas del Evento: 31/03/2019 - 05/04/2019
Lugar del Evento: Cracovia, Polonia
Título del Libro: Proceedings of 13th European Conference on Antennas and Propagation (EuCAP 2019)
Fecha: Agosto 2019
ISBN: 9781538681275
Materias:
ODS:
Palabras Clave Informales: Frequency Selective Surfaces; Inductive FSS;Dichroic; Cassegrain; Intertwined
Escuela: E.T.S.I. Telecomunicación (UPM)
Departamento: Señales, Sistemas y Radiocomunicaciones
Licencias Creative Commons: Reconocimiento - Sin obra derivada - No comercial

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Resumen

An intertwined tri-band Inductive Frequency Selective Surface (FSS) configured as Cassegrain sub-reflector for Earth to Satellite communication is presented. The sub-reflectoris designed to provide linear polarization independency and maximum transparency to electromagnetic waves in K and Ka band at frequencies 16.4-20.4 GHz and 28.2-32.5 GHz respectively, and provide maximum reflectivity to electromagnetic waves in K band at frequencies 23.6-25.4 GHz. The sub-reflector is designed using the Jerusalem cross element along with an intertwined shape. The intertwine shape will reduce the second resonant frequency as well as given more angular stability and maximum bandwidth. The transmission and reflection parameters are shown in all frequencies of interest. Finally, the full structure will be simulated as a flat sub-reflector and placed at the front of horn antennas working at the centre of the frequency bands to compare the radiation pattern agains the classical Cassegrain and prime focus configurations. The simulation are carried out using CST Microwave Studio.

Proyectos asociados

Tipo
Código
Acrónimo
Responsable
Título
Gobierno de España
TEC2017-85529-C3-1-R
FUTURE-RADIO
Sin especificar
Radio systems and technologies for high capacity terrestrial and satellite communications in an hyperconnected world
Comunidad de Madrid
S2013/ICE-3000
SPADERADAR-CM
Sin especificar
Space Debris Radar- Radar para detección de basura espacial

Más información

ID de Registro: 64538
Identificador DC: https://oa.upm.es/64538/
Identificador OAI: oai:oa.upm.es:64538
URL Oficial: https://www.eucap2019.org/
Depositado por: Memoria Investigacion
Depositado el: 01 Mar 2021 14:37
Ultima Modificación: 30 Ene 2025 14:02