Published October 12, 2004
| Published
Book Section - Chapter
Open
Planck-HFI focal plane concept
Chicago
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 | Download all |
---|---|---|
md5:bf61e268fc9e34c537c43184b1217c03
|
631.2 kB | Preview Download |
Additional details
- Eprint ID
- 93121
- Resolver ID
- CaltechAUTHORS:20190221-110525411
- Created
-
2019-02-25Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 5487