Published 2014 | Version v1
Journal article

Low Loss Superconducting Microstrip Development at Argonne National Lab

  • 1. University of Chicago, IL (United States). Kavli Institute for Cosmological Physics. Dept. of Astronomy and Astrophysics
  • 2. Argonne National Laboratory (ANL), Argonne, IL (United States). High-Energy Physics Division
  • 3. Cardiff University (United Kingdom). School of Physics and Astronomy
  • 4. SLAC National Accelerator Laboratory, Menlo Park, CA (United States)
  • 5. Stanford University, CA (United States). Kavli Institute for Particle Astrophysics and Cosmology. Dept. of Physics

Description

Low loss superconducting microstrip is an essential component in realizing 100 kilo-pixel multichroic cosmic microwave background detector arrays. In this paper, we have been developing a low loss microstrip by understanding and controlling the loss mechanisms. We present the fabrication of the superconducting microstrip, the loss measurements at a few GHz frequencies using half-wavelength resonators, and the loss measurements at 220 GHz frequencies with the superconducting microstrip coupled to slot antennas at one end and to TES detectors at the other end. Finally, the measured loss tangent of the microstrip made of sputtered Nb and SiOx is 1-2e-3.

Availability note (English)

Available from http://www.osti.gov/pages/servlets/purl/1357457; http://www.osti.gov/pages/biblio/1357457; DOE Accepted Manuscript full text, or the publishers Best Available Version will be available free of charge after the embargo period

Additional details

Publishing Information

Journal Title
IEEE Transactions on Applied Superconductivity (Print)
Journal Volume
25
Journal Issue
3
Journal Page Range
vp.
ISSN
1051-8223