Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/7865
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dc.contributor.authorRao, K.B. Raghavendra-
dc.contributor.authorT.S., Mamatha-
dc.contributor.authorDeshpande, A.A.-
dc.date.accessioned2021-12-15T08:24:01Z-
dc.date.available2021-12-15T08:24:01Z-
dc.date.issued2016-05-27-
dc.identifier.citationRRI-EEG Internal Technical Report No. : 3en_US
dc.identifier.urihttp://hdl.handle.net/2289/7865-
dc.descriptionRestricted Accessen_US
dc.description.abstractObserving the radio sky at low frequencies, particularly in sites where FM signal and other RFI dominates, is highly challenging, since the radio receiver is prone to be driven to saturation by these strong signals. So it is required that the receiver should have high dynamic range and / or very low sensitivity to FM signal for proper observation. We have developed a low- noise amplifier with about 40 dB rejection to the FM signal, in the frequency range of 50 – 500 MHz for use in the Sky Watch Array Network (SWAN). It has a noise temperature ranging from 40-80 K, a gain of 20 dB with a variation of ± 1.5 dB around the band center and around 60 dB dynamic range over the specified band. The design details and test results are presented in this report.en_US
dc.language.isoenen_US
dc.publisherRaman Research Institute, Bengaluruen_US
dc.rights2016 Raman Research Institute, Bengaluruen_US
dc.title50 – 500 MHz Low Noise Amplifier with FM band rejectionen_US
dc.typeTechnical Reporten_US
Appears in Collections:Technical Reports (EEG)

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