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Proceedings Paper

New RF data on ECCOSORB CR/MF absorber
Author(s): L. Valenziano; O. A. Peverini; M. Zannoni; R. Tascone; G. Addamo; G. Virone; M. Lumia; S. Mariotti; A. De Rosa
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Paper Abstract

ECCOSORBTM CR/MF is a widely used absorber at radio and millimeter wavelengths. It is used both at room and at cryogenic temperature to realize loads and calibrators both for laboratory and for space-borne instruments. Data on its RF properties are available from the data sheet at room temperature. But it is also widely used outside the design wavelength range and at cryogenic temperature, where specific measurement of electromagnetic and thermal properties are needed. Scarce information is available in the literature and inconsistencies are frequent. We report here new RF data in Ka and W-band at room temperature obtained with waveguide measurements with different setups.

Paper Details

Date Published: 23 July 2014
PDF: 7 pages
Proc. SPIE 9153, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII, 91532X (23 July 2014); doi: 10.1117/12.2056315
Show Author Affiliations
L. Valenziano, Istituto Nazionale di AstroFisica Spaziale e Fisica Cosmica (Italy)
O. A. Peverini, Istituto di Elettronica, Computer e Ingegneria delle Telecomunicazioni, CNR (Italy)
M. Zannoni, Univ. degli Studi di Milano-Bicocca (Italy)
R. Tascone, Istituto di Elettronica, Computer e Ingegneria delle Telecomunicazioni, CNR (Italy)
G. Addamo, Istituto di Elettronica, Computer e Ingegneria delle Telecomunicazioni, CNR (Italy)
G. Virone, Istituto di Elettronica, Computer e Ingegneria delle Telecomunicazioni, CNR (Italy)
M. Lumia, Istituto di Elettronica, Computer e Ingegneria delle Telecomunicazioni, CNR (Italy)
S. Mariotti, INAF - Istituto di Radioastronomia (Italy)
A. De Rosa, INAF - Istituto Nazionale di AstroFisica Spaziale e Fisica Cosmica (Italy)


Published in SPIE Proceedings Vol. 9153:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)

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