1974
DOI: 10.21236/ad0783433
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A Study of the Measurement of G/T Using Cassiopeia A

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Cited by 9 publications
(15 citation statements)
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“…(1) The noise-add standard source with its power supply, which is attached to the crossguide coupler at the antenna low-noise amplifier input; (2) the ETMS control/rf console which plugs into the IF patch panel (this unit also requires two coaxial cables which go up to the antenna rf-plate to remotely control the noise-add source); (3) the power-detector unit which is a thermally-isolated commercial thermistor mount and an NBS type IV power-meter; (4) the multi-channel input digital-voltmeter which measures and digitizes the various measurement parameters and monitor voltages in the system; (5) the clock which provides time information to the calculator for predicting star locations; (6) temperature/dew point monitor for calculating water absorption corrections to the star flux,…”
Section: Softwarementioning
confidence: 99%
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“…(1) The noise-add standard source with its power supply, which is attached to the crossguide coupler at the antenna low-noise amplifier input; (2) the ETMS control/rf console which plugs into the IF patch panel (this unit also requires two coaxial cables which go up to the antenna rf-plate to remotely control the noise-add source); (3) the power-detector unit which is a thermally-isolated commercial thermistor mount and an NBS type IV power-meter; (4) the multi-channel input digital-voltmeter which measures and digitizes the various measurement parameters and monitor voltages in the system; (5) the clock which provides time information to the calculator for predicting star locations; (6) temperature/dew point monitor for calculating water absorption corrections to the star flux,…”
Section: Softwarementioning
confidence: 99%
“…Unpacking and Inspection Temperature/dew point probe enclosure 3 cartons printer paper (6 Type "ENTER (3,*) M,T"…”
Section: 2mentioning
confidence: 99%
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“…Present typical accuracies of measurement of antenna gain are about 1 dB, but errors of several dB are not uncommon [ 5 ] . The estimated uncertainty to be achieved by OSP and its support NBSES will be in the vicinity of 0.1 to 0.2 dB.…”
Section: Impact Upon System Investment and Operating Costsmentioning
confidence: 99%
“…Their functions, which are not critical to the subject of this report, will be addressed and discussed only as necessary to the understanding of the actual measurement process and its verification. We show in Figure 4 (4) Nature of services to be offered; (5) Frequency and band coverages; (6) Hardware design; (7) Payload allocations to equipment, fuel, etc., and (8) moon to measure G/T of an earth-station [5] . The advantages of using radio stars to determine G/T are: The "signal" level is low, and not suitable for sidelobe evaluation.…”
mentioning
confidence: 99%