CaltechAUTHORS
Published October 12, 2004 | Version Published
Book Section - Chapter Open

Planck-HFI focal plane concept

Creators

  • 1. ROR icon Cardiff University
  • 2. ROR icon Jet Propulsion Lab
  • 3. ROR icon Centre National d'Études Spatiales
  • 4. ROR icon National University of Ireland, Maynooth
  • 5. ROR icon Paris Observatory
  • 6. ROR icon California Institute of Technology
  • 7. ROR icon University of Paris-Saclay

Contributors

Abstract

The future ESA space mission Planck Surveyor mission will measure the Cosmic Microwave Background temperature and polarisation anisotropies in a frequency domain comprised between 30GHz and 1THz. On board two instruments, LFI based on HEMT technology and HFI using bolometric detectors. We present the optical solutions adopted for this mission, in particular the focal plane design of HFI, concept which has been applied already to other instruments such as the balloon borne experiment Archeops.

Additional Information

© 2004 Society of Photo-Optical Instrumentation Engineers (SPIE).

Attached Files

Published - 523.pdf

Files

523.pdf

Files (631.2 kB)

Name Size
md5:bf61e268fc9e34c537c43184b1217c03
631.2 kB Preview Download

Additional details

Identifiers

Eprint ID
93121
Resolver ID
CaltechAUTHORS:20190221-110525411

Dates

Created
2019-02-25
Created from EPrint's datestamp field
Updated
2021-11-16
Created from EPrint's last_modified field

Caltech Custom Metadata

Caltech groups
Physics Department
Series Name
Proceedings of SPIE
Series Volume or Issue Number
5487