{"title":"Phase characterization of the meteor burst channel","authors":"K. Parsa, D. Schilling","doi":"10.1109/MILCOM.1991.258300","DOIUrl":null,"url":null,"abstract":"A necessary step in the design of high-speed adaptive meteor burst (MB) systems is to determine how the channel distorts the phase of the meteor signal. This aspect of the meteor burst channels is characterized. An enhanced MB channel model is developed. This is achieved by characterizing the MB Doppler spread, Doppler rate, head-echo induced phase jitter, and deriving simple mathematical expressions for them.<<ETX>>","PeriodicalId":212388,"journal":{"name":"MILCOM 91 - Conference record","volume":"8 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1991-11-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"MILCOM 91 - Conference record","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/MILCOM.1991.258300","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
A necessary step in the design of high-speed adaptive meteor burst (MB) systems is to determine how the channel distorts the phase of the meteor signal. This aspect of the meteor burst channels is characterized. An enhanced MB channel model is developed. This is achieved by characterizing the MB Doppler spread, Doppler rate, head-echo induced phase jitter, and deriving simple mathematical expressions for them.<>
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