E. Choi, J. Anderson, J. Sirigiri, M. Shapiro, R. Temkin
{"title":"具有非均匀电子发射的1.5 MW, 110 GHz MIT回旋管的MAGY模拟","authors":"E. Choi, J. Anderson, J. Sirigiri, M. Shapiro, R. Temkin","doi":"10.1109/IVELEC.2004.1316355","DOIUrl":null,"url":null,"abstract":"We present simulation results from the code MAGY of a 110 GHz, 1.5 MW gyrotron which is currently in short pulse operation at MIT. The experimental peak power is 1.44 MW at 37 % efficiency, when operating in the TE/sub 22,6/ mode, with a velocity ratio (v/sub /spl perp///v/sub /spl par//) of 1.43. The MAGY simulations are done for triplet mode excitation (TE/sub 21,6/, TE/sub 22,6/ and TE/sub 23,6/), and include both velocity spread and the azimuthal nonuniform charge density of the electron beam. For a velocity spread of 5.5 % and the measured value of beam emission nonuniformity, the MAGY simulations are in good agreement with the measured experimental results.","PeriodicalId":283559,"journal":{"name":"Fifth IEEE International Vacuum Electronics Conference (IEEE Cat. No.04EX786)","volume":"1 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2004-04-27","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":"{\"title\":\"MAGY simulations of 1.5 MW, 110 GHz MIT gyrotron with non-uniform electron emission\",\"authors\":\"E. Choi, J. Anderson, J. Sirigiri, M. Shapiro, R. Temkin\",\"doi\":\"10.1109/IVELEC.2004.1316355\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"We present simulation results from the code MAGY of a 110 GHz, 1.5 MW gyrotron which is currently in short pulse operation at MIT. The experimental peak power is 1.44 MW at 37 % efficiency, when operating in the TE/sub 22,6/ mode, with a velocity ratio (v/sub /spl perp///v/sub /spl par//) of 1.43. The MAGY simulations are done for triplet mode excitation (TE/sub 21,6/, TE/sub 22,6/ and TE/sub 23,6/), and include both velocity spread and the azimuthal nonuniform charge density of the electron beam. For a velocity spread of 5.5 % and the measured value of beam emission nonuniformity, the MAGY simulations are in good agreement with the measured experimental results.\",\"PeriodicalId\":283559,\"journal\":{\"name\":\"Fifth IEEE International Vacuum Electronics Conference (IEEE Cat. No.04EX786)\",\"volume\":\"1 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2004-04-27\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"1\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Fifth IEEE International Vacuum Electronics Conference (IEEE Cat. No.04EX786)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/IVELEC.2004.1316355\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Fifth IEEE International Vacuum Electronics Conference (IEEE Cat. No.04EX786)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/IVELEC.2004.1316355","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
MAGY simulations of 1.5 MW, 110 GHz MIT gyrotron with non-uniform electron emission
We present simulation results from the code MAGY of a 110 GHz, 1.5 MW gyrotron which is currently in short pulse operation at MIT. The experimental peak power is 1.44 MW at 37 % efficiency, when operating in the TE/sub 22,6/ mode, with a velocity ratio (v/sub /spl perp///v/sub /spl par//) of 1.43. The MAGY simulations are done for triplet mode excitation (TE/sub 21,6/, TE/sub 22,6/ and TE/sub 23,6/), and include both velocity spread and the azimuthal nonuniform charge density of the electron beam. For a velocity spread of 5.5 % and the measured value of beam emission nonuniformity, the MAGY simulations are in good agreement with the measured experimental results.