Loading…
Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders
Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirem...
Saved in:
Main Authors: | , , , , |
---|---|
Format: | Conference Proceeding |
Language: | English |
Subjects: | |
Online Access: | Request full text |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
cited_by | |
---|---|
cites | |
container_end_page | |
container_issue | |
container_start_page | 265 |
container_title | |
container_volume | |
creator | Saraph, G.P. Lawson, W. Anderson, J.P. Castle, M. Granatstein, V.L. |
description | Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity. |
doi_str_mv | 10.1109/PLASMA.1996.551515 |
format | conference_proceeding |
fullrecord | <record><control><sourceid>osti_6IE</sourceid><recordid>TN_cdi_ieee_primary_551515</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><ieee_id>551515</ieee_id><sourcerecordid>435465</sourcerecordid><originalsourceid>FETCH-LOGICAL-i113t-9ca1f8ae6d83ef66df752176d58bfaed066342dd044e1e6277eaa9e0cf5c54da3</originalsourceid><addsrcrecordid>eNotkEtLAzEcxIMPsNR-gZ7ival5Z_dYSn3gFgUV9bSkyT81ut0tyXrot3elzgz8LsMcBqEpo3PGaHn9VC2e14s5K0s9V4oNPkEjrowmhtPiFE1KU9AhQgjO-RkaUSMoKbmUF2iS8xcdJBUTgo7QxyqE6CK0_QwzSgnTFK_fZvidYNt6_PBDNn_cHlL33Rxyn7oW292-iSFCwh5y3LYZhy7hJrZgE3Zd00QPKV-i82CbDJN_jtHrzepleUeqx9v75aIikTHRk9JZFgoL2hcCgtY-GMWZ0V4Vm2DBU62F5N5TKYGB5saAtSVQF5RT0lsxRlfH3S73sc4u9uA-Xde24PpaCiW1GjrTYycCQL1PcWfToT5-J34B3O1few</addsrcrecordid><sourcetype>Open Access Repository</sourcetype><iscdi>true</iscdi><recordtype>conference_proceeding</recordtype></control><display><type>conference_proceeding</type><title>Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders</title><source>IEEE Electronic Library (IEL) Conference Proceedings</source><creator>Saraph, G.P. ; Lawson, W. ; Anderson, J.P. ; Castle, M. ; Granatstein, V.L.</creator><creatorcontrib>Saraph, G.P. ; Lawson, W. ; Anderson, J.P. ; Castle, M. ; Granatstein, V.L.</creatorcontrib><description>Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity.</description><identifier>ISSN: 0730-9244</identifier><identifier>ISBN: 9780780333222</identifier><identifier>ISBN: 0780333225</identifier><identifier>EISSN: 2576-7208</identifier><identifier>DOI: 10.1109/PLASMA.1996.551515</identifier><language>eng</language><publisher>United States: IEEE</publisher><subject>CAVITY RESONATORS ; COMPUTERIZED SIMULATION ; Cyclotrons ; DESIGN ; Dielectric losses ; Klystrons ; LINEAR COLLIDERS ; Magnetic fields ; MICROWAVE AMPLIFIERS ; PARTICLE ACCELERATORS ; Plasma simulation ; Plasma sources ; POWER RANGE 100-1000 MW ; Pulse amplifiers ; Q factor ; Scattering parameters ; Stability</subject><ispartof>IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science, 1996, p.265</ispartof><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://ieeexplore.ieee.org/document/551515$$EHTML$$P50$$Gieee$$H</linktohtml><link.rule.ids>230,309,310,780,784,789,790,885,2058,4050,4051,23930,27925,54555,54920,54932</link.rule.ids><linktorsrc>$$Uhttps://ieeexplore.ieee.org/document/551515$$EView_record_in_IEEE$$FView_record_in_$$GIEEE</linktorsrc><backlink>$$Uhttps://www.osti.gov/biblio/435465$$D View this record in Osti.gov$$Hfree_for_read</backlink></links><search><creatorcontrib>Saraph, G.P.</creatorcontrib><creatorcontrib>Lawson, W.</creatorcontrib><creatorcontrib>Anderson, J.P.</creatorcontrib><creatorcontrib>Castle, M.</creatorcontrib><creatorcontrib>Granatstein, V.L.</creatorcontrib><title>Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders</title><title>IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science</title><addtitle>PLASMA</addtitle><description>Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity.</description><subject>CAVITY RESONATORS</subject><subject>COMPUTERIZED SIMULATION</subject><subject>Cyclotrons</subject><subject>DESIGN</subject><subject>Dielectric losses</subject><subject>Klystrons</subject><subject>LINEAR COLLIDERS</subject><subject>Magnetic fields</subject><subject>MICROWAVE AMPLIFIERS</subject><subject>PARTICLE ACCELERATORS</subject><subject>Plasma simulation</subject><subject>Plasma sources</subject><subject>POWER RANGE 100-1000 MW</subject><subject>Pulse amplifiers</subject><subject>Q factor</subject><subject>Scattering parameters</subject><subject>Stability</subject><issn>0730-9244</issn><issn>2576-7208</issn><isbn>9780780333222</isbn><isbn>0780333225</isbn><fulltext>true</fulltext><rsrctype>conference_proceeding</rsrctype><creationdate>1996</creationdate><recordtype>conference_proceeding</recordtype><sourceid>6IE</sourceid><recordid>eNotkEtLAzEcxIMPsNR-gZ7ival5Z_dYSn3gFgUV9bSkyT81ut0tyXrot3elzgz8LsMcBqEpo3PGaHn9VC2e14s5K0s9V4oNPkEjrowmhtPiFE1KU9AhQgjO-RkaUSMoKbmUF2iS8xcdJBUTgo7QxyqE6CK0_QwzSgnTFK_fZvidYNt6_PBDNn_cHlL33Rxyn7oW292-iSFCwh5y3LYZhy7hJrZgE3Zd00QPKV-i82CbDJN_jtHrzepleUeqx9v75aIikTHRk9JZFgoL2hcCgtY-GMWZ0V4Vm2DBU62F5N5TKYGB5saAtSVQF5RT0lsxRlfH3S73sc4u9uA-Xde24PpaCiW1GjrTYycCQL1PcWfToT5-J34B3O1few</recordid><startdate>1996</startdate><enddate>1996</enddate><creator>Saraph, G.P.</creator><creator>Lawson, W.</creator><creator>Anderson, J.P.</creator><creator>Castle, M.</creator><creator>Granatstein, V.L.</creator><general>IEEE</general><general>Institute of Electrical and Electronics Engineers, Inc., Piscataway, NJ (United States)</general><scope>6IE</scope><scope>6IL</scope><scope>CBEJK</scope><scope>RIE</scope><scope>RIL</scope><scope>OTOTI</scope></search><sort><creationdate>1996</creationdate><title>Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders</title><author>Saraph, G.P. ; Lawson, W. ; Anderson, J.P. ; Castle, M. ; Granatstein, V.L.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-i113t-9ca1f8ae6d83ef66df752176d58bfaed066342dd044e1e6277eaa9e0cf5c54da3</frbrgroupid><rsrctype>conference_proceedings</rsrctype><prefilter>conference_proceedings</prefilter><language>eng</language><creationdate>1996</creationdate><topic>CAVITY RESONATORS</topic><topic>COMPUTERIZED SIMULATION</topic><topic>Cyclotrons</topic><topic>DESIGN</topic><topic>Dielectric losses</topic><topic>Klystrons</topic><topic>LINEAR COLLIDERS</topic><topic>Magnetic fields</topic><topic>MICROWAVE AMPLIFIERS</topic><topic>PARTICLE ACCELERATORS</topic><topic>Plasma simulation</topic><topic>Plasma sources</topic><topic>POWER RANGE 100-1000 MW</topic><topic>Pulse amplifiers</topic><topic>Q factor</topic><topic>Scattering parameters</topic><topic>Stability</topic><toplevel>online_resources</toplevel><creatorcontrib>Saraph, G.P.</creatorcontrib><creatorcontrib>Lawson, W.</creatorcontrib><creatorcontrib>Anderson, J.P.</creatorcontrib><creatorcontrib>Castle, M.</creatorcontrib><creatorcontrib>Granatstein, V.L.</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><collection>OSTI.GOV</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Saraph, G.P.</au><au>Lawson, W.</au><au>Anderson, J.P.</au><au>Castle, M.</au><au>Granatstein, V.L.</au><format>book</format><genre>proceeding</genre><ristype>CONF</ristype><atitle>Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders</atitle><btitle>IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science</btitle><stitle>PLASMA</stitle><date>1996</date><risdate>1996</risdate><spage>265</spage><pages>265-</pages><issn>0730-9244</issn><eissn>2576-7208</eissn><isbn>9780780333222</isbn><isbn>0780333225</isbn><abstract>Summary form only given. Efficient, 100-160 MW, X- and Ku-band microwave sources with pulse-lengths of 1 /spl mu/s are being developed for driving future linear colliders. Two-cavity and three-cavity, co-axial designs of relativistic gyroklystron amplifiers are presented which fulfill these requirements. Simulations are carried out using the existing set of codes which includes a scattering matrix code for cold-cavity fields, a linear start-oscillation code for stability, and a nonlinear gyroklystron code for optimizing parameters to get maximum efficiency and gain. The cavities are designed to have high mode purity, good inter-cavity isolation, and stability to the excitation of the spurious modes. The quality factors of the cavities, the lengths of the drift sections, and the magnetic field profile are optimized for each design. During this study, the effect of velocity spread in the beam on the efficiency of the device is taken into account. In addition, HFSS code is used to study the effect of dielectric loading and power losses in the cavity.</abstract><cop>United States</cop><pub>IEEE</pub><doi>10.1109/PLASMA.1996.551515</doi></addata></record> |
fulltext | fulltext_linktorsrc |
identifier | ISSN: 0730-9244 |
ispartof | IEEE Conference Record - Abstracts. 1996 IEEE International Conference on Plasma Science, 1996, p.265 |
issn | 0730-9244 2576-7208 |
language | eng |
recordid | cdi_ieee_primary_551515 |
source | IEEE Electronic Library (IEL) Conference Proceedings |
subjects | CAVITY RESONATORS COMPUTERIZED SIMULATION Cyclotrons DESIGN Dielectric losses Klystrons LINEAR COLLIDERS Magnetic fields MICROWAVE AMPLIFIERS PARTICLE ACCELERATORS Plasma simulation Plasma sources POWER RANGE 100-1000 MW Pulse amplifiers Q factor Scattering parameters Stability |
title | Efficient, 100-160 MW, X- and Ku-band gyroklystron amplifier designs for linear colliders |
url | http://sfxeu10.hosted.exlibrisgroup.com/loughborough?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-02T20%3A44%3A44IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-osti_6IE&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=proceeding&rft.atitle=Efficient,%20100-160%20MW,%20X-%20and%20Ku-band%20gyroklystron%20amplifier%20designs%20for%20linear%20colliders&rft.btitle=IEEE%20Conference%20Record%20-%20Abstracts.%201996%20IEEE%20International%20Conference%20on%20Plasma%20Science&rft.au=Saraph,%20G.P.&rft.date=1996&rft.spage=265&rft.pages=265-&rft.issn=0730-9244&rft.eissn=2576-7208&rft.isbn=9780780333222&rft.isbn_list=0780333225&rft_id=info:doi/10.1109/PLASMA.1996.551515&rft_dat=%3Costi_6IE%3E435465%3C/osti_6IE%3E%3Cgrp_id%3Ecdi_FETCH-LOGICAL-i113t-9ca1f8ae6d83ef66df752176d58bfaed066342dd044e1e6277eaa9e0cf5c54da3%3C/grp_id%3E%3Coa%3E%3C/oa%3E%3Curl%3E%3C/url%3E&rft_id=info:oai/&rft_id=info:pmid/&rft_ieee_id=551515&rfr_iscdi=true |