Cryogenic 3 mm Schottky diode mixer receiver
The best cooled Schottky diode mixer receivers at mm and submm wavelengths use specially fabricated "cryogenic" diodes. Parameters of these diodes permit one to realize very low noise temperatures when cryocooled, the noise temperature of the UVA2P9-600 diode being less than 50 K at 20 K)....
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creator | Peskovatskii, S.A. Shulga, V.M. Piddiachii, V.I. Koroliov, A.M. Myshenko, V.V. Antuyfeyev, A.V. Lavrik, I.V. |
description | The best cooled Schottky diode mixer receivers at mm and submm wavelengths use specially fabricated "cryogenic" diodes. Parameters of these diodes permit one to realize very low noise temperatures when cryocooled, the noise temperature of the UVA2P9-600 diode being less than 50 K at 20 K). Preliminary investigation at 20 K of the I-V characteristics of the available diodes has shown them possessing the noise temperature theoretical limit of about 110 K. This is considerably higher than the noise of the above-mentioned "cryogenic" diode UVA2P9-600. With the purpose of compensating this high level of Schottky diode noise, we have focused our efforts on the reduction of the mixer conversion loss. Our receiver design incorporates a full-height waveguide mixer mount employing no input guide impedance transformer, thus reducing the waveguide channel and backshort losses. The necessary input impedance transformation in this mixer mount is realized immediately at the Schottky diode location. The DSB receiver noise temperature with a full-height waveguide mixer at room temperature is 270 K. For cryogenic operation an overmoded waveguide and linear taper to rectangular waveguide are added to the receiver input circuit. |
doi_str_mv | 10.1109/MSMW.2001.947295 |
format | Conference Proceeding |
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Parameters of these diodes permit one to realize very low noise temperatures when cryocooled, the noise temperature of the UVA2P9-600 diode being less than 50 K at 20 K). Preliminary investigation at 20 K of the I-V characteristics of the available diodes has shown them possessing the noise temperature theoretical limit of about 110 K. This is considerably higher than the noise of the above-mentioned "cryogenic" diode UVA2P9-600. With the purpose of compensating this high level of Schottky diode noise, we have focused our efforts on the reduction of the mixer conversion loss. Our receiver design incorporates a full-height waveguide mixer mount employing no input guide impedance transformer, thus reducing the waveguide channel and backshort losses. The necessary input impedance transformation in this mixer mount is realized immediately at the Schottky diode location. The DSB receiver noise temperature with a full-height waveguide mixer at room temperature is 270 K. For cryogenic operation an overmoded waveguide and linear taper to rectangular waveguide are added to the receiver input circuit.</description><identifier>ISBN: 9780780364738</identifier><identifier>ISBN: 0780364732</identifier><identifier>DOI: 10.1109/MSMW.2001.947295</identifier><language>eng</language><publisher>IEEE</publisher><subject>Circuit noise ; Cryogenics ; Impedance ; Low-frequency noise ; Noise level ; Noise measurement ; Receivers ; Rectangular waveguides ; Schottky diodes ; Temperature measurement</subject><ispartof>Fourth International Kharkov Symposium 'Physics and Engineering of Millimeter and Sub-Millimeter Waves'. Symposium Proceedings (Cat. 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Symposium Proceedings (Cat. No.01EX429)</title><addtitle>MSMW</addtitle><description>The best cooled Schottky diode mixer receivers at mm and submm wavelengths use specially fabricated "cryogenic" diodes. Parameters of these diodes permit one to realize very low noise temperatures when cryocooled, the noise temperature of the UVA2P9-600 diode being less than 50 K at 20 K). Preliminary investigation at 20 K of the I-V characteristics of the available diodes has shown them possessing the noise temperature theoretical limit of about 110 K. This is considerably higher than the noise of the above-mentioned "cryogenic" diode UVA2P9-600. With the purpose of compensating this high level of Schottky diode noise, we have focused our efforts on the reduction of the mixer conversion loss. Our receiver design incorporates a full-height waveguide mixer mount employing no input guide impedance transformer, thus reducing the waveguide channel and backshort losses. The necessary input impedance transformation in this mixer mount is realized immediately at the Schottky diode location. The DSB receiver noise temperature with a full-height waveguide mixer at room temperature is 270 K. For cryogenic operation an overmoded waveguide and linear taper to rectangular waveguide are added to the receiver input circuit.</description><subject>Circuit noise</subject><subject>Cryogenics</subject><subject>Impedance</subject><subject>Low-frequency noise</subject><subject>Noise level</subject><subject>Noise measurement</subject><subject>Receivers</subject><subject>Rectangular waveguides</subject><subject>Schottky diodes</subject><subject>Temperature measurement</subject><isbn>9780780364738</isbn><isbn>0780364732</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>2001</creationdate><recordtype>conference_proceeding</recordtype><sourceid>6IE</sourceid><sourceid>RIE</sourceid><recordid>eNotj09LxDAUxAMiKGvv4ikfwNa8JG3eO0rxH-ziYRc8LjF51ai1khax397C7jAwlx8zjBCXoCoARTeb7eal0kpBRdZpqk9EQQ7VYtNYZ_BMFOP4oRYZqhHxXFy3eR7e-DsFaWTfy214H6bpc5YxDZFln_44y8yB0y_nC3Ha-a-Ri2OuxO7-btc-luvnh6f2dl0mpKlk7T3o1-AoBOosN9AEBqpNRI-GlmUXgaBB9EFbs0C6A-VrT5EbS9qsxNWhNjHz_ien3ud5f3hk_gFhOj_z</recordid><startdate>2001</startdate><enddate>2001</enddate><creator>Peskovatskii, S.A.</creator><creator>Shulga, V.M.</creator><creator>Piddiachii, V.I.</creator><creator>Koroliov, A.M.</creator><creator>Myshenko, V.V.</creator><creator>Antuyfeyev, A.V.</creator><creator>Lavrik, I.V.</creator><general>IEEE</general><scope>6IE</scope><scope>6IL</scope><scope>CBEJK</scope><scope>RIE</scope><scope>RIL</scope></search><sort><creationdate>2001</creationdate><title>Cryogenic 3 mm Schottky diode mixer receiver</title><author>Peskovatskii, S.A. ; Shulga, V.M. ; Piddiachii, V.I. ; Koroliov, A.M. ; Myshenko, V.V. ; Antuyfeyev, A.V. ; Lavrik, I.V.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i89t-e2aa12bc79cc9f4e616ce1953d8a8393957d191688ac243cc92f10a5a9de64923</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>2001</creationdate><topic>Circuit noise</topic><topic>Cryogenics</topic><topic>Impedance</topic><topic>Low-frequency noise</topic><topic>Noise level</topic><topic>Noise measurement</topic><topic>Receivers</topic><topic>Rectangular waveguides</topic><topic>Schottky diodes</topic><topic>Temperature measurement</topic><toplevel>online_resources</toplevel><creatorcontrib>Peskovatskii, S.A.</creatorcontrib><creatorcontrib>Shulga, V.M.</creatorcontrib><creatorcontrib>Piddiachii, V.I.</creatorcontrib><creatorcontrib>Koroliov, A.M.</creatorcontrib><creatorcontrib>Myshenko, V.V.</creatorcontrib><creatorcontrib>Antuyfeyev, A.V.</creatorcontrib><creatorcontrib>Lavrik, I.V.</creatorcontrib><collection>IEEE Electronic Library (IEL) Conference Proceedings</collection><collection>IEEE Proceedings Order Plan All Online (POP All Online) 1998-present by volume</collection><collection>IEEE Xplore All Conference Proceedings</collection><collection>IEEE Electronic Library (IEL)</collection><collection>IEEE Proceedings Order Plans (POP All) 1998-Present</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Peskovatskii, S.A.</au><au>Shulga, V.M.</au><au>Piddiachii, V.I.</au><au>Koroliov, A.M.</au><au>Myshenko, V.V.</au><au>Antuyfeyev, A.V.</au><au>Lavrik, I.V.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Cryogenic 3 mm Schottky diode mixer receiver</atitle><btitle>Fourth International Kharkov Symposium 'Physics and Engineering of Millimeter and Sub-Millimeter Waves'. Symposium Proceedings (Cat. No.01EX429)</btitle><stitle>MSMW</stitle><date>2001</date><risdate>2001</risdate><volume>2</volume><spage>741</spage><epage>743 vol.2</epage><pages>741-743 vol.2</pages><isbn>9780780364738</isbn><isbn>0780364732</isbn><abstract>The best cooled Schottky diode mixer receivers at mm and submm wavelengths use specially fabricated "cryogenic" diodes. Parameters of these diodes permit one to realize very low noise temperatures when cryocooled, the noise temperature of the UVA2P9-600 diode being less than 50 K at 20 K). Preliminary investigation at 20 K of the I-V characteristics of the available diodes has shown them possessing the noise temperature theoretical limit of about 110 K. This is considerably higher than the noise of the above-mentioned "cryogenic" diode UVA2P9-600. With the purpose of compensating this high level of Schottky diode noise, we have focused our efforts on the reduction of the mixer conversion loss. Our receiver design incorporates a full-height waveguide mixer mount employing no input guide impedance transformer, thus reducing the waveguide channel and backshort losses. The necessary input impedance transformation in this mixer mount is realized immediately at the Schottky diode location. The DSB receiver noise temperature with a full-height waveguide mixer at room temperature is 270 K. For cryogenic operation an overmoded waveguide and linear taper to rectangular waveguide are added to the receiver input circuit.</abstract><pub>IEEE</pub><doi>10.1109/MSMW.2001.947295</doi></addata></record> |
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identifier | ISBN: 9780780364738 |
ispartof | Fourth International Kharkov Symposium 'Physics and Engineering of Millimeter and Sub-Millimeter Waves'. Symposium Proceedings (Cat. No.01EX429), 2001, Vol.2, p.741-743 vol.2 |
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language | eng |
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source | IEEE Electronic Library (IEL) Conference Proceedings |
subjects | Circuit noise Cryogenics Impedance Low-frequency noise Noise level Noise measurement Receivers Rectangular waveguides Schottky diodes Temperature measurement |
title | Cryogenic 3 mm Schottky diode mixer receiver |
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