{"title":"Evaluation of the ionospheric noise and variability within the hour by 5 minutes ionospheric soundings","authors":"B. Zolesi , S.S. Kouris , D. Fotiadis , C. Scotto","doi":"10.1016/S1464-1917(01)00013-7","DOIUrl":null,"url":null,"abstract":"<div><p>The actual future needs in radio propagation predictions are short-term ionospheric forecasting and now-casting. These are often given at standard hours, but in order to improve the reliability and the accuracy of forecasting, the variability within-the-hour and the so-called “intrinsic noise” of the ionosphere cannot be neglected anymore. Values of <em>f</em><sub>o</sub>F2 and MUF(3000)F2, obtained in 5-minutes vertical sounding campaigns, performed at Rome and Juliusruh ionospheric stations during different seasons and different levels of solar activity, are analysed and the results are discussed.</p></div>","PeriodicalId":101026,"journal":{"name":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","volume":"26 5","pages":"Pages 359-362"},"PeriodicalIF":0.0000,"publicationDate":"2001-01-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/S1464-1917(01)00013-7","citationCount":"2","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Physics and Chemistry of the Earth, Part C: Solar, Terrestrial & Planetary Science","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1464191701000137","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 2
Abstract
The actual future needs in radio propagation predictions are short-term ionospheric forecasting and now-casting. These are often given at standard hours, but in order to improve the reliability and the accuracy of forecasting, the variability within-the-hour and the so-called “intrinsic noise” of the ionosphere cannot be neglected anymore. Values of foF2 and MUF(3000)F2, obtained in 5-minutes vertical sounding campaigns, performed at Rome and Juliusruh ionospheric stations during different seasons and different levels of solar activity, are analysed and the results are discussed.