电离层效应早于2003年10月的万圣节风暴

D. Blagoveshchensky, J. MacDougall, A. V. Pyatkova
{"title":"电离层效应早于2003年10月的万圣节风暴","authors":"D. Blagoveshchensky, J. MacDougall, A. V. Pyatkova","doi":"10.1109/RAST.2005.1512667","DOIUrl":null,"url":null,"abstract":"The goal of this study is to reveal some ionospheric forerunners which occur prior to the expansion phase of any storm or substorm. Another task is to compare variations of two main ionospheric parameters, f/sub 0/F2 and h/sub max/F2, on two chains of ionosondes located in Europe and North America during the interval October 16-28, 2003. This interval precedes the Halloween storm and includes its onset. Analysis is based on ionospheric data of the SPIDR system. The key findings are as follows. A positive peak of delta f/sub 0/F2 occurs some hours before onset of a magnetic storm or substorm, where delta is a deviation from the quiet value. This peak can serve as a forerunner of disturbance development. Delta f/sub 0/F2 peak amplitude reaches the sizes 20-100% of f/sub 0/F2 values. Similarities of delta f/sub 0/F2 variations on two chains are: (i) the delta f/sub 0/F2 peak mentioned above occurs simultaneously as a rule before disturbances on both chains; (ii) similar delta f/sub 0/F2 variations are observed on all of the mid-latitude (or high-latitude) ionosondes of each of the chain. Delta h/sub max/F2 variations are approximately the opposite of the f/sub 0/F2 variations. Their amplitudes fall in the range 15 - 25% from the average h/sub max/F2 value. This investigation is useful and important for the short-term prediction of space weather states.","PeriodicalId":156704,"journal":{"name":"Proceedings of 2nd International Conference on Recent Advances in Space Technologies, 2005. RAST 2005.","volume":"73 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2005-06-09","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Ionospheric effects preceded the October 2003 Halloween storm\",\"authors\":\"D. Blagoveshchensky, J. MacDougall, A. V. Pyatkova\",\"doi\":\"10.1109/RAST.2005.1512667\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"The goal of this study is to reveal some ionospheric forerunners which occur prior to the expansion phase of any storm or substorm. Another task is to compare variations of two main ionospheric parameters, f/sub 0/F2 and h/sub max/F2, on two chains of ionosondes located in Europe and North America during the interval October 16-28, 2003. This interval precedes the Halloween storm and includes its onset. Analysis is based on ionospheric data of the SPIDR system. The key findings are as follows. A positive peak of delta f/sub 0/F2 occurs some hours before onset of a magnetic storm or substorm, where delta is a deviation from the quiet value. This peak can serve as a forerunner of disturbance development. Delta f/sub 0/F2 peak amplitude reaches the sizes 20-100% of f/sub 0/F2 values. Similarities of delta f/sub 0/F2 variations on two chains are: (i) the delta f/sub 0/F2 peak mentioned above occurs simultaneously as a rule before disturbances on both chains; (ii) similar delta f/sub 0/F2 variations are observed on all of the mid-latitude (or high-latitude) ionosondes of each of the chain. Delta h/sub max/F2 variations are approximately the opposite of the f/sub 0/F2 variations. Their amplitudes fall in the range 15 - 25% from the average h/sub max/F2 value. This investigation is useful and important for the short-term prediction of space weather states.\",\"PeriodicalId\":156704,\"journal\":{\"name\":\"Proceedings of 2nd International Conference on Recent Advances in Space Technologies, 2005. RAST 2005.\",\"volume\":\"73 1\",\"pages\":\"0\"},\"PeriodicalIF\":0.0000,\"publicationDate\":\"2005-06-09\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Proceedings of 2nd International Conference on Recent Advances in Space Technologies, 2005. RAST 2005.\",\"FirstCategoryId\":\"1085\",\"ListUrlMain\":\"https://doi.org/10.1109/RAST.2005.1512667\",\"RegionNum\":0,\"RegionCategory\":null,\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"\",\"JCRName\":\"\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Proceedings of 2nd International Conference on Recent Advances in Space Technologies, 2005. RAST 2005.","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1109/RAST.2005.1512667","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0

摘要

本研究的目的是揭示在任何风暴或亚风暴扩张阶段之前发生的一些电离层前兆。另一项任务是比较2003年10月16日至28日期间位于欧洲和北美的两条电离层探测链上的两个主要电离层参数f/sub 0/F2和h/sub max/F2的变化。这个间隔在万圣节风暴之前,包括它的开始。分析基于SPIDR系统的电离层数据。主要发现如下。δ f/ δ 0/F2的正峰值出现在磁暴或亚暴开始前的几个小时,其中δ是与安静值的偏差。这个峰值可以作为扰动发展的先兆。δ f/sub 0/F2峰值振幅达到f/sub 0/F2值的20-100%。两条链上f/sub 0/F2变化的相似之处是:(i)上述f/sub 0/F2峰通常同时出现在两条链上的扰动之前;(ii)在每条链的所有中纬度(或高纬度)电离空探空仪上观测到类似的δ f/sub 0/F2变化。h/sub max/F2的变化与f/sub 0/F2的变化大致相反。它们的振幅从平均h/sub max/F2值下降15 - 25%。这一研究对空间天气状态的短期预报具有重要意义。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Ionospheric effects preceded the October 2003 Halloween storm
The goal of this study is to reveal some ionospheric forerunners which occur prior to the expansion phase of any storm or substorm. Another task is to compare variations of two main ionospheric parameters, f/sub 0/F2 and h/sub max/F2, on two chains of ionosondes located in Europe and North America during the interval October 16-28, 2003. This interval precedes the Halloween storm and includes its onset. Analysis is based on ionospheric data of the SPIDR system. The key findings are as follows. A positive peak of delta f/sub 0/F2 occurs some hours before onset of a magnetic storm or substorm, where delta is a deviation from the quiet value. This peak can serve as a forerunner of disturbance development. Delta f/sub 0/F2 peak amplitude reaches the sizes 20-100% of f/sub 0/F2 values. Similarities of delta f/sub 0/F2 variations on two chains are: (i) the delta f/sub 0/F2 peak mentioned above occurs simultaneously as a rule before disturbances on both chains; (ii) similar delta f/sub 0/F2 variations are observed on all of the mid-latitude (or high-latitude) ionosondes of each of the chain. Delta h/sub max/F2 variations are approximately the opposite of the f/sub 0/F2 variations. Their amplitudes fall in the range 15 - 25% from the average h/sub max/F2 value. This investigation is useful and important for the short-term prediction of space weather states.
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
自引率
0.00%
发文量
0
×
引用
GB/T 7714-2015
复制
MLA
复制
APA
复制
导出至
BibTeX EndNote RefMan NoteFirst NoteExpress
×
提示
您的信息不完整,为了账户安全,请先补充。
现在去补充
×
提示
您因"违规操作"
具体请查看互助需知
我知道了
×
提示
确定
请完成安全验证×
copy
已复制链接
快去分享给好友吧!
我知道了
右上角分享
点击右上角分享
0
联系我们:info@booksci.cn Book学术提供免费学术资源搜索服务,方便国内外学者检索中英文文献。致力于提供最便捷和优质的服务体验。 Copyright © 2023 布克学术 All rights reserved.
京ICP备2023020795号-1
ghs 京公网安备 11010802042870号
Book学术文献互助
Book学术文献互助群
群 号:481959085
Book学术官方微信