A cryogenic rotation stage with a large clear aperture for the half-wave plates in the Spider instrument.

نویسندگان

  • Sean Bryan
  • Peter Ade
  • Mandana Amiri
  • Steven Benton
  • Richard Bihary
  • James Bock
  • J Richard Bond
  • H Cynthia Chiang
  • Carlo Contaldi
  • Brendan Crill
  • Olivier Dore
  • Benjamin Elder
  • Jeffrey Filippini
  • Aurelien Fraisse
  • Anne Gambrel
  • Natalie Gandilo
  • Jon Gudmundsson
  • Matthew Hasselfield
  • Mark Halpern
  • Gene Hilton
  • Warren Holmes
  • Viktor Hristov
  • Kent Irwin
  • William Jones
  • Zigmund Kermish
  • Craig Lawrie
  • Carrie MacTavish
  • Peter Mason
  • Krikor Megerian
  • Lorenzo Moncelsi
  • Thomas Montroy
  • Tracy Morford
  • Johanna Nagy
  • C Barth Netterfield
  • Ivan Padilla
  • Alexandra S Rahlin
  • Carl Reintsema
  • Daniel C Riley
  • John Ruhl
  • Marcus Runyan
  • Benjamin Saliwanchik
  • Jamil Shariff
  • Juan Soler
  • Amy Trangsrud
  • Carole Tucker
  • Rebecca Tucker
  • Anthony Turner
  • Shyang Wen
  • Donald Wiebe
  • Edward Young
چکیده

We describe the cryogenic half-wave plate rotation mechanisms built for and used in Spider, a polarization-sensitive balloon-borne telescope array that observed the cosmic microwave background at 95 GHz and 150 GHz during a stratospheric balloon flight from Antarctica in January 2015. The mechanisms operate at liquid helium temperature in flight. A three-point contact design keeps the mechanical bearings relatively small but allows for a large (305 mm) diameter clear aperture. A worm gear driven by a cryogenic stepper motor allows for precise positioning and prevents undesired rotation when the motors are depowered. A custom-built optical encoder system monitors the bearing angle to an absolute accuracy of ±0.1(∘). The system performed well in Spider during its successful 16 day flight.

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عنوان ژورنال:
  • The Review of scientific instruments

دوره 87 1  شماره 

صفحات  -

تاریخ انتشار 2016