{"title":"通过三维射线追踪研究了土星射电闪电的“超越地平线”传播","authors":"A.-L. Gautier, B. Cecconi, P. Zarka, G. Fischer","doi":"10.1109/URSIGASS.2011.6051302","DOIUrl":null,"url":null,"abstract":"Saturn Electrostatic Discharges (SED] are radio signature of lightning flashes originating from Saturns cloud systems. Observations of SED show that the radio horizon is larger than the visible one, especially when Cassini is in Saturns morning side (“over the horizon” effect]. Moreover, both apparition and disappearance of bursts appear to be frequency-dependent. We built a 3D ray tracing code, which computes the path propagation of radio waves through a realistic model of Saturns ionosphere, where electron density varies with local time, and were able to reproduce the typical dynamic spectrum of observed “over the horizon” events.","PeriodicalId":325870,"journal":{"name":"2011 XXXth URSI General Assembly and Scientific Symposium","volume":"63 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2011-10-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Propagation “over the horizon” of Saturn's radio lightning studied by three-dimensional ray tracing\",\"authors\":\"A.-L. Gautier, B. Cecconi, P. Zarka, G. Fischer\",\"doi\":\"10.1109/URSIGASS.2011.6051302\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Saturn Electrostatic Discharges (SED] are radio signature of lightning flashes originating from Saturns cloud systems. Observations of SED show that the radio horizon is larger than the visible one, especially when Cassini is in Saturns morning side (“over the horizon” effect]. Moreover, both apparition and disappearance of bursts appear to be frequency-dependent. We built a 3D ray tracing code, which computes the path propagation of radio waves through a realistic model of Saturns ionosphere, where electron density varies with local time, and were able to reproduce the typical dynamic spectrum of observed “over the horizon” events.\",\"PeriodicalId\":325870,\"journal\":{\"name\":\"2011 XXXth URSI General Assembly and Scientific Symposium\",\"volume\":\"63 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2011-10-20\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2011 XXXth URSI General Assembly and Scientific Symposium\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/URSIGASS.2011.6051302\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2011 XXXth URSI General Assembly and Scientific Symposium","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/URSIGASS.2011.6051302","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Propagation “over the horizon” of Saturn's radio lightning studied by three-dimensional ray tracing
Saturn Electrostatic Discharges (SED] are radio signature of lightning flashes originating from Saturns cloud systems. Observations of SED show that the radio horizon is larger than the visible one, especially when Cassini is in Saturns morning side (“over the horizon” effect]. Moreover, both apparition and disappearance of bursts appear to be frequency-dependent. We built a 3D ray tracing code, which computes the path propagation of radio waves through a realistic model of Saturns ionosphere, where electron density varies with local time, and were able to reproduce the typical dynamic spectrum of observed “over the horizon” events.