Optical requirements and modelling of coupling devices for the SAFARI instrument on SPICA

N. Trappe, J. R. Gao, D. Glowacka, D. Goldie, D. Griffin, P. Khosropanah, P. Mauskopf, D. Morozov, A. Murphy, C. O'Sullivan, M. Ridder, S. Withington

Research output: Chapter in Book/Report/Conference proceedingConference contribution

1 Scopus citations

Abstract

The next generation of space missions targeting far-infrared bands will require large-format arrays of extremely low-noise detectors. The development of Transition Edge Sensors (TES) array technology seems to be a viable solution for future mm-wave to Far-Infrared (FIR) space applications where low noise and high sensitivity is required. In this paper we concentrate on a key element for a high sensitivity TES detector array, that of the optical coupling between the incoming electromagnetic field and the phonon system of the suspended membrane. An intermediate solution between free space coupling and a single moded horn is where over-moded light pipes are used to concentrate energy onto multi-moded absorbers. We present a comparison of modelling techniques to analyse the optical efficiency of such light pipes and their interaction with the front end optics and detector cavity.

Original languageEnglish (US)
Title of host publicationProceedings of the 5th European Conference on Antennas and Propagation, EUCAP 2011
Pages3321-3324
Number of pages4
StatePublished - Jul 1 2011
Externally publishedYes
Event5th European Conference on Antennas and Propagation, EUCAP 2011 - Rome, Italy
Duration: Apr 10 2011Apr 15 2011

Publication series

NameProceedings of the 5th European Conference on Antennas and Propagation, EUCAP 2011

Other

Other5th European Conference on Antennas and Propagation, EUCAP 2011
Country/TerritoryItaly
CityRome
Period4/10/114/15/11

ASJC Scopus subject areas

  • Hardware and Architecture
  • Electrical and Electronic Engineering

Fingerprint

Dive into the research topics of 'Optical requirements and modelling of coupling devices for the SAFARI instrument on SPICA'. Together they form a unique fingerprint.

Cite this