The Herschel -Heterodyne Instrument for the Far-Infrared (HIFI)
Leiden University · Atacama Large Millimeter Submillimeter Array · +36 more institutions
Abstract
Aims. This paper describes the Heterodyne Instrument for the Far-Infrared (HIFI) that was launched onboard ESA's Herschel Space Observatory in May 2009. Methods. The instrument is a set of 7 heterodyne receivers that are electronically tuneable, covering 480–1250 GHz with SIS mixers and the 1410–1910 GHz range with hot electron bolometer (HEB) mixers. The local oscillator (LO) subsystem comprises a Ka-band synthesizer followed by 14 chains of frequency multipliers and 2 chains for each frequency band. A pair of auto-correlators and a pair of acousto-optical spectrometers process the two IF signals from the dual-polarization, single-pixel front-ends to provide instantaneous frequency coverage of 2 × 4 GHz, with…
Citation impact
- FWCI
- 61.96
- Percentile
- 100%
- References
- 5
Authors
166- TDTh. de GraauwCorresponding
Leiden University, Atacama Large Millimeter Submillimeter Array, Leiden Observatory, Space Research Organisation Netherlands
- FHF. Helmich
Space Research Organisation Netherlands
- TGT. G. Phillips
California Institute of Technology
- JSJ. Stützki
University of Cologne
- ECE. Caux
Centre National de la Recherche Scientifique, Université Toulouse III - Paul Sabatier, Université Fédérale de Toulouse Midi-Pyrénées
Topics & keywords
- Physics
- Heterodyne (poetry)
- Superheterodyne receiver
- Bolometer
- Local oscillator
- Optics
- Spectrometer
- Intermediate frequency
Funding
- NANational Aeronautics and Space Administration
- CICalifornia Institute of Technology
- EIEnterprise Ireland
- CNCentre National d’Etudes Spatiales
- NONederlandse Organisatie voor Wetenschappelijk Onderzoek
- ASAgenzia Spaziale Italiana
- KOKnut och Alice Wallenbergs Stiftelse
- CNCentre National de la Recherche Scientifique
- INIstituto Nazionale di Astrofisica
- MDMinisterio de Fomento
- CSCanadian Space Agency
- INInstitut national des sciences de l'Univers