{"title":"Observations of radio wave phase characteristics on a high-frequency auroral path","authors":"J. Koch, W. Beery","doi":"10.6028/JRES.066D.033","DOIUrl":null,"url":null,"abstract":"Experimental observations of phase perturbations to continuous wave and pulse signals, over short time periods, have been carried out on a high-frequency auroral path. Statistics on phase perturbations occurring in time intervals of one to twent y milliseconds were obtained for t he continuous wave signals. Pulse-to-pulse phase stability measurements were made, using one-millisecond pulses with a pulse repetition rate of 250 pulses per second. The phase of corresponding parts of successive pulses were compared continuously, and then t he integrated values of phase differences during one-millisecond pulse periods were deter mined. Comparisons of statistics of phase perturbations for continuous wave signals and one-millisecond pulse signals indicate no significant differences for approximately four millisecond sampli ng intervals and comparable fading speeds on t his auroral path.","PeriodicalId":398550,"journal":{"name":"Journal of Research of the National Bureau of Standards, Section D: Radio Propagation","volume":"352 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"1962-05-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Research of the National Bureau of Standards, Section D: Radio Propagation","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.6028/JRES.066D.033","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
Experimental observations of phase perturbations to continuous wave and pulse signals, over short time periods, have been carried out on a high-frequency auroral path. Statistics on phase perturbations occurring in time intervals of one to twent y milliseconds were obtained for t he continuous wave signals. Pulse-to-pulse phase stability measurements were made, using one-millisecond pulses with a pulse repetition rate of 250 pulses per second. The phase of corresponding parts of successive pulses were compared continuously, and then t he integrated values of phase differences during one-millisecond pulse periods were deter mined. Comparisons of statistics of phase perturbations for continuous wave signals and one-millisecond pulse signals indicate no significant differences for approximately four millisecond sampli ng intervals and comparable fading speeds on t his auroral path.