Juan Yi, XuDong Gu, Wen Cheng, XinYue Tang, Long Chen, BinBin Ni, RuoXian Zhou, ZhengYu Zhao, Qi Wang, LiQing Zhou
{"title":"WHU ELF/VLF接收机低纬度周大气观测的详细研究:1。发生特征及相关电离层参数","authors":"Juan Yi, XuDong Gu, Wen Cheng, XinYue Tang, Long Chen, BinBin Ni, RuoXian Zhou, ZhengYu Zhao, Qi Wang, LiQing Zhou","doi":"10.26464/epp2020023","DOIUrl":null,"url":null,"abstract":"<p>As a companion paper to Zhou RX et al. (2020), this study describes application of the automatic detection and analysis module to identify all the tweek atmospherics detectible in the WHU ELF/VLF receiver data collected at Suizhou station during the period of 3 February through 29 February 2016. Detailed analysis of the identified low-latitude tweek events reveals that the occurrence rate varies considerably — from 800 to 6000 tweeks per day, and exhibits a strong diurnal and local time dependence, the peak occurring before local midnight. The diurnal variation of identified tweeks was similar to that of the lightning data obtained by the World-Wide Lightning Location Network (WWLLN).. Estimates of the propagation distance and ionospheric reflection height of tweek atmospherics suggest that the majority (~92%) of the low latitude tweeks originate from the lightning activity within a radius of 4000 km and that they are very likely to reflect from the lower ionospheric D-region at the height range of 75–85 km. At these lower ionospheric reflection altitudes, ~74% of the corresponding electron densities from the tweek spectral measurements are within 24.5–27.5 cm <sup>-3</sup>. The daily variation of estimated D-region electron densities in the considered period (February 2016) also exhibits a small overall increasing trend from early to later in the month.</p>","PeriodicalId":45246,"journal":{"name":"Earth and Planetary Physics","volume":"4 3","pages":"238-245"},"PeriodicalIF":1.9000,"publicationDate":"2020-06-08","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.26464/epp2020023","citationCount":"9","resultStr":"{\"title\":\"A detailed investigation of low latitude tweek atmospherics observed by the WHU ELF/VLF receiver: 2. Occurrence features and associated ionospheric parameters\",\"authors\":\"Juan Yi, XuDong Gu, Wen Cheng, XinYue Tang, Long Chen, BinBin Ni, RuoXian Zhou, ZhengYu Zhao, Qi Wang, LiQing Zhou\",\"doi\":\"10.26464/epp2020023\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>As a companion paper to Zhou RX et al. (2020), this study describes application of the automatic detection and analysis module to identify all the tweek atmospherics detectible in the WHU ELF/VLF receiver data collected at Suizhou station during the period of 3 February through 29 February 2016. Detailed analysis of the identified low-latitude tweek events reveals that the occurrence rate varies considerably — from 800 to 6000 tweeks per day, and exhibits a strong diurnal and local time dependence, the peak occurring before local midnight. The diurnal variation of identified tweeks was similar to that of the lightning data obtained by the World-Wide Lightning Location Network (WWLLN).. Estimates of the propagation distance and ionospheric reflection height of tweek atmospherics suggest that the majority (~92%) of the low latitude tweeks originate from the lightning activity within a radius of 4000 km and that they are very likely to reflect from the lower ionospheric D-region at the height range of 75–85 km. At these lower ionospheric reflection altitudes, ~74% of the corresponding electron densities from the tweek spectral measurements are within 24.5–27.5 cm <sup>-3</sup>. The daily variation of estimated D-region electron densities in the considered period (February 2016) also exhibits a small overall increasing trend from early to later in the month.</p>\",\"PeriodicalId\":45246,\"journal\":{\"name\":\"Earth and Planetary Physics\",\"volume\":\"4 3\",\"pages\":\"238-245\"},\"PeriodicalIF\":1.9000,\"publicationDate\":\"2020-06-08\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"https://sci-hub-pdf.com/10.26464/epp2020023\",\"citationCount\":\"9\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Earth and Planetary Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://onlinelibrary.wiley.com/doi/10.26464/epp2020023\",\"RegionNum\":3,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Earth and Planetary Physics","FirstCategoryId":"89","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.26464/epp2020023","RegionNum":3,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 9
摘要
作为Zhou RX等人(2020)的合作论文,本研究描述了在2016年2月3日至2月29日期间随州站收集的WHU ELF/VLF接收机数据中,应用自动检测和分析模块识别可检测的所有两周大气。对已确定的低纬度双周事件的详细分析表明,其发生率变化很大,从每天800到6000双周不等,并且表现出强烈的日和当地时间依赖性,高峰发生在当地午夜之前。所识别的两周的日变化与世界闪电定位网(WWLLN)获得的闪电数据相似。对两周大气传播距离和电离层反射高度的估计表明,低纬度两周大气的大部分(~92%)来自4000 km半径内的闪电活动,它们很可能在75 ~ 85 km高度范围内从较低的电离层d区反射。在这些较低的电离层反射高度,从两周光谱测量得到的~74%的相应电子密度在24.5-27.5 cm -3范围内。在考虑的时间段内(2016年2月),估计的d区电子密度的日变化也呈现出从月初到月末的小幅度整体增加趋势。
A detailed investigation of low latitude tweek atmospherics observed by the WHU ELF/VLF receiver: 2. Occurrence features and associated ionospheric parameters
As a companion paper to Zhou RX et al. (2020), this study describes application of the automatic detection and analysis module to identify all the tweek atmospherics detectible in the WHU ELF/VLF receiver data collected at Suizhou station during the period of 3 February through 29 February 2016. Detailed analysis of the identified low-latitude tweek events reveals that the occurrence rate varies considerably — from 800 to 6000 tweeks per day, and exhibits a strong diurnal and local time dependence, the peak occurring before local midnight. The diurnal variation of identified tweeks was similar to that of the lightning data obtained by the World-Wide Lightning Location Network (WWLLN).. Estimates of the propagation distance and ionospheric reflection height of tweek atmospherics suggest that the majority (~92%) of the low latitude tweeks originate from the lightning activity within a radius of 4000 km and that they are very likely to reflect from the lower ionospheric D-region at the height range of 75–85 km. At these lower ionospheric reflection altitudes, ~74% of the corresponding electron densities from the tweek spectral measurements are within 24.5–27.5 cm -3. The daily variation of estimated D-region electron densities in the considered period (February 2016) also exhibits a small overall increasing trend from early to later in the month.