1967
DOI: 10.1016/0003-4916(67)90179-0
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Measurement of cosmic background radiation at 3.2-cm wavelength

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1968
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Cited by 13 publications
(1 citation statement)
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“…The underlying approach explored in this work for baseline removal has its roots in a variety of analogous instruments such as frequency-swept reflectometry 25 and spectral baseline correction in radio astronomy. 26,27 In particular, the differential reflectometer configuration used for cavity characterization 28 provides insight in this context. In this method, the baseline is explicitly removed on resonance by comparing the response of a waveguide cavity with that of a short-circuit via the difference port of a magic-T power divider.…”
Section: Measurement Metrology Motivationmentioning
confidence: 99%
“…The underlying approach explored in this work for baseline removal has its roots in a variety of analogous instruments such as frequency-swept reflectometry 25 and spectral baseline correction in radio astronomy. 26,27 In particular, the differential reflectometer configuration used for cavity characterization 28 provides insight in this context. In this method, the baseline is explicitly removed on resonance by comparing the response of a waveguide cavity with that of a short-circuit via the difference port of a magic-T power divider.…”
Section: Measurement Metrology Motivationmentioning
confidence: 99%