Abstract
Bolometers are used as detectors in the Herschel SPIRE and PACS instruments. This chapter focuses on the history of bolometer development leading to the SPIRE and PACS detectors, operating in the submillimetre and far-infrared wavelength ranges. This historical and technological review describes the main technical lineages of bolometers and how the SPIRE and PACS instruments on Herschel, respectively, employed both an adapted and improved variant of a well-established technology and a novel bolometer architecture developed especially for the mission.
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Notes
- 1.
NEFD is the overall NEP divided by the aperture area of the telescope, the bandwidth of the instrument, the atmospheric transmission if on earth, and various parameters characterising the optics transmission and coupling to incident radiation . In astronomy, it is often expressed in terms of Jansky (Jy) with 1 Jy = 10–26 W m–2 Hz–1.
- 2.
Aperture efficiency is defined as the fraction of the power from a point source that is coupled to the detector by the optical system.
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Minier, V. et al. (2017). Far-Infrared Bolometers: Technical Lineages. In: Inventing a Space Mission. ISSI Scientific Report Series, vol 14. Springer, Cham. https://doi.org/10.1007/978-3-319-60024-6_7
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