太阳x耀斑极大期太阳氢Lyα线发射对电离层d区总电离率的贡献

IF 0.8 4区物理与天体物理 Q4 ASTRONOMY & ASTROPHYSICS

Serbian Astronomical Journal Pub Date : 2015-12-01 DOI:10.2298/SAJ150828003N

A. Nina, V. M. vCadevz, J. Bajvceti'c

{"title":"太阳x耀斑极大期太阳氢Lyα线发射对电离层d区总电离率的贡献","authors":"A. Nina, V. M. vCadevz, J. Bajvceti'c","doi":"10.2298/SAJ150828003N","DOIUrl":null,"url":null,"abstract":"The solar Lyα line emission can be considered as the dominant source of \n ionization processes in the ionospheric D-region at altitudes above 70 km \n during unperturbed conditions. However, large sudden impacts of radiation in \n some other energy domains can also significantly influence the ionization \n rate and, in this paper, we present a study on the contribution of Lyα \n radiation to the ionization rate when the ionosphere is disturbed by solar \n X-flares. We give relevant analytical expressions and make calculations and \n numerical simulations for the low ionosphere using data collected by the VLF \n receiver located in Serbia for the VLF radio signal emitted by the DHO \n transmitter in Germany. [Projekat Ministarstva nauke Republike Srbije, br. \n III-44002, br. 176002 i br. 176004]","PeriodicalId":48878,"journal":{"name":"Serbian Astronomical Journal","volume":"191 1","pages":"51-57"},"PeriodicalIF":0.8000,"publicationDate":"2015-12-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"2","resultStr":"{\"title\":\"Contribution of solar hydrogen Lyα line emission in total ionization rate in ionospheric D-region during the maximum of solar X-flare\",\"authors\":\"A. Nina, V. M. vCadevz, J. Bajvceti'c\",\"doi\":\"10.2298/SAJ150828003N\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The solar Lyα line emission can be considered as the dominant source of \\n ionization processes in the ionospheric D-region at altitudes above 70 km \\n during unperturbed conditions. However, large sudden impacts of radiation in \\n some other energy domains can also significantly influence the ionization \\n rate and, in this paper, we present a study on the contribution of Lyα \\n radiation to the ionization rate when the ionosphere is disturbed by solar \\n X-flares. We give relevant analytical expressions and make calculations and \\n numerical simulations for the low ionosphere using data collected by the VLF \\n receiver located in Serbia for the VLF radio signal emitted by the DHO \\n transmitter in Germany. [Projekat Ministarstva nauke Republike Srbije, br. \\n III-44002, br. 176002 i br. 176004]\",\"PeriodicalId\":48878,\"journal\":{\"name\":\"Serbian Astronomical Journal\",\"volume\":\"191 1\",\"pages\":\"51-57\"},\"PeriodicalIF\":0.8000,\"publicationDate\":\"2015-12-01\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"2\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Serbian Astronomical Journal\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://doi.org/10.2298/SAJ150828003N\",\"RegionNum\":4,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q4\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Serbian Astronomical Journal","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.2298/SAJ150828003N","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q4","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}

引用次数: 2

摘要

在无扰动条件下，太阳Lyα线发射可以被认为是海拔70 km以上电离层d区电离过程的主要来源。然而，在一些其他能量域的辐射的大的突然影响也可以显著地影响电离率，在本文中，我们提出了一个研究Lyα辐射对电离率的贡献，当电离层受到太阳x耀斑的干扰。利用位于塞尔维亚的VLF接收机采集的数据，对德国DHO发射机发射的VLF无线电信号进行了低电离层的计算和数值模拟。[南斯拉夫]塞族共和国部长项目;3 - 44002, br。[176002 .]176004]

本文章由计算机程序翻译，如有差异，请以英文原文为准。

查看原文本刊更多论文

Contribution of solar hydrogen Lyα line emission in total ionization rate in ionospheric D-region during the maximum of solar X-flare

The solar Lyα line emission can be considered as the dominant source of ionization processes in the ionospheric D-region at altitudes above 70 km during unperturbed conditions. However, large sudden impacts of radiation in some other energy domains can also significantly influence the ionization rate and, in this paper, we present a study on the contribution of Lyα radiation to the ionization rate when the ionosphere is disturbed by solar X-flares. We give relevant analytical expressions and make calculations and numerical simulations for the low ionosphere using data collected by the VLF receiver located in Serbia for the VLF radio signal emitted by the DHO transmitter in Germany. [Projekat Ministarstva nauke Republike Srbije, br. III-44002, br. 176002 i br. 176004]

求助全文

通过发布文献求助，成功后即可免费获取论文全文。去求助

来源期刊

Serbian Astronomical Journal ASTRONOMY & ASTROPHYSICS-

CiteScore

1.00

自引率

0.00%

发文量

审稿时长

12 weeks

期刊介绍： Serbian Astronomical Journal publishes original observations and researches in all branches of astronomy. The journal publishes: Invited Reviews - review article on some up-to-date topic in astronomy, astrophysics and related fields (written upon invitation only), Original Scientific Papers - article in which are presented previously unpublished author''s own scientific results, Preliminary Reports - original scientific paper, but shorter in length and of preliminary nature, Professional Papers - articles offering experience useful for the improvement of professional practice i.e. article describing methods and techniques, software, presenting observational data, etc. In some cases the journal may publish other contributions, such as In Memoriam notes, Obituaries, Book Reviews, as well as Editorials, Addenda, Errata, Corrigenda, Retraction notes, etc.