A. Maxworth, G. Hussey, K. McWilliams, A. Yau, Gordon James
{"title":"e-POP-RRI观测到的哨声及其相关现象","authors":"A. Maxworth, G. Hussey, K. McWilliams, A. Yau, Gordon James","doi":"10.23919/USNC/URSI49741.2020.9321633","DOIUrl":null,"url":null,"abstract":"In this work, we present observations from the Radio Receiver Instrument (RRI) on the enhanced Polar Outflow Probe (e-POP, also known as SWARM-E). We have observed whistlers, proton whistlers, hiss and chorus. The observed polarization parameters, were used to determine the proton gyrofrequencies and cross-over frequencies. These parameters were compared against the modeled values from the IGRF model.","PeriodicalId":443426,"journal":{"name":"2020 IEEE USNC-CNC-URSI North American Radio Science Meeting (Joint with AP-S Symposium)","volume":"35 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-07-05","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Whistlers and Related Phenomenon Observed by e-POP-RRI\",\"authors\":\"A. Maxworth, G. Hussey, K. McWilliams, A. Yau, Gordon James\",\"doi\":\"10.23919/USNC/URSI49741.2020.9321633\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"In this work, we present observations from the Radio Receiver Instrument (RRI) on the enhanced Polar Outflow Probe (e-POP, also known as SWARM-E). We have observed whistlers, proton whistlers, hiss and chorus. The observed polarization parameters, were used to determine the proton gyrofrequencies and cross-over frequencies. These parameters were compared against the modeled values from the IGRF model.\",\"PeriodicalId\":443426,\"journal\":{\"name\":\"2020 IEEE USNC-CNC-URSI North American Radio Science Meeting (Joint with AP-S Symposium)\",\"volume\":\"35 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2020-07-05\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"2020 IEEE USNC-CNC-URSI North American Radio Science Meeting (Joint with AP-S Symposium)\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.23919/USNC/URSI49741.2020.9321633\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"2020 IEEE USNC-CNC-URSI North American Radio Science Meeting (Joint with AP-S Symposium)","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.23919/USNC/URSI49741.2020.9321633","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
Whistlers and Related Phenomenon Observed by e-POP-RRI
In this work, we present observations from the Radio Receiver Instrument (RRI) on the enhanced Polar Outflow Probe (e-POP, also known as SWARM-E). We have observed whistlers, proton whistlers, hiss and chorus. The observed polarization parameters, were used to determine the proton gyrofrequencies and cross-over frequencies. These parameters were compared against the modeled values from the IGRF model.