The Planck-LFI flight model composite waveguides
O. D'Arcangelo, L. Figini, A. Simonetto, F.Villa, M. Pecora, P., Battaglia, M. Bersanelli, R.C. Butler, F. Cuttaia, S. Garavaglia, P. Guzzi,, N. Mandolesi, A. Mennella, G. Morgante, L. Pagan, L. Valenziano

TL;DR
This paper details the design, manufacturing, and testing of composite waveguides for the Planck-LFI instrument, ensuring they meet thermal, electromagnetic, and mechanical requirements for space application.
Contribution
It presents the development and space qualification of complex composite waveguides tailored for the Planck satellite's low-frequency instrument.
Findings
Waveguides meet all electromagnetic and mechanical requirements.
Successful space qualification of the composite waveguides.
Manufacturing process optimized for complex shapes and length.
Abstract
The Low Frequency Instrument on board the PLANCK satellite is designed to give the most accurate map ever of the CMB anisotropy of the whole sky over a broad frequency band spanning 27 to 77 GHz. It is made of an array of 22 pseudo-correlation radiometers, composed of 11 actively cooled (20 K) Front End Modules (FEMs), and 11 Back End Modules (BEMs) at 300K. The connection between the two parts is made with rectangular Wave Guides. Considerations of different nature (thermal, electromagnetic and mechanical), imposed stringent requirements on the WGs characteristics and drove their design. From the thermal point of view, the WG should guarantee good insulation between the FEM and the BEM sections to avoid overloading the cryocooler. On the other hand it is essential that the signals do not undergo excessive attenuation through the WG. Finally, given the different positions of the FEM…
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