2014Unpublished venueRequires access

Heterodyne receivers for high frequency THz astrophysics

Heinz‐Wilhelm Hübers

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Abstract

The performance of heterodyne receivers for frequencies beyond 1.4 THz will be reviewed. Emphasis will be on the development of the 4.7-THz frequency channel for the GREAT heterodyne spectrometer on SOFIA. This receiver is based on a phonon-cooled hot-electron bolometric mixer and a quantum-cascade laser as local oscillator.

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What this paper is about

The performance of heterodyne receivers for frequencies beyond 1.4 THz will be reviewed. Emphasis will be on the development of the 4.7-THz frequency channel for the GREAT heterodyne spectrometer on SOFIA. This receiver is based on a phonon-cooled hot-electron bolometric mixer and a quantum-cascade laser as local oscillator.

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Available abstract

The performance of heterodyne receivers for frequencies beyond 1.4 THz will be reviewed. Emphasis will be on the development of the 4.7-THz frequency channel for the GREAT heterodyne spectrometer on SOFIA. This receiver is based on a phonon-cooled hot-electron bolometric mixer and a quantum-cascade laser as local oscillator.

Key concepts: Superheterodyne receiver, Terahertz radiation, Heterodyne (poetry), Local oscillator, Quantum cascade laser, Bolometer, Physics, Intermediate frequency

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