Solar and geomagnetic activity dependence of 150-km echoes observed by the Equatorial Atmosphere Radar in Indonesia
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DOI[10.1186/s40623-022-01675-6]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Tatsuhiro YokoyamaRieko TakagiMamoru Yamamoto
- Publication, Distribution, etc.
- Publication Date
- 2022-07-22
- Publication Date (W3CDTF)
- 2022-07-22
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 74(113)
- Volume
- 74(113)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-022-01675-6
- Persistent ID (NDL)
- info:ndljp/pid/12685400
- Collection
- Collection (Materials For Handicapped People:1)
- Collection (particular)
- 国立国会図書館デジタルコレクション > 電子書籍・電子雑誌 > その他
- Acquisition Basis
- オンライン資料収集制度
- Date Accepted (W3CDTF)
- 2023-03-07T16:17:01+09:00
- Date Captured (W3CDTF)
- 2023-03-07
- Format (IMT)
- application/pdf
- Access Restrictions
- 国立国会図書館内限定公開
- Service for the Digitized Contents Transmission Service
- 図書館・個人送信対象外
- Availability of remote photoduplication service
- 可
- Periodical Title (URI)
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/12287068
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館デジタルコレクション
- Summary, etc.
- The occurrence characteristics of 150-km echoes in low-latitude regions are studied using the Equatorial Atmosphere Radar (EAR) in Indonesia. The long-term observation of the 150-km echoes by the EAR enables us to study the occurrence characteristics of 150-km echoes statistically. It is shown that the occurrence rate of the 150-km echoes observed by the EAR shows a semiannual variation with two peaks in solstices and a negative correlation with both the EUV flux and ΣKp index, that is, the solar and the geomagnetic activity. Geomagnetic activity correlates with the occurrence rate of 150-km echoes observed one day after when the ΣKp was measured. However, the occurrence rate is always low during the high solar activity period regardless of the geomagnetic activity. While the seasonal variation and the solar activity dependence of the occurrence of 150-km echoes are consistent with previous studies, this is the first time a negative correlation with geomagnetic activity is reported.
- DOI
- 10.1186/s40623-022-01675-6
- Access Restrictions
- インターネット公開
- Rights (production)
- © The Author(s) 2022This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder.
- Related Material (URI)
- Is Referenced By
- Solved and unsolved riddles about low-latitude daytime valley region plasma waves and 150-km echoes
- References
- The Solar Flux Dependence of Ionospheric 150 km Radar Echoes and ImplicationsOn the Solstice Maxima and Azimuth‐Dependent Characteristics of the 150‐km Echoes Observed Using the Equatorial Atmosphere RadarDaytime zonal drifts in the ionospheric 150 km and <i>E</i> regions estimated using EAR observationsStatistics of 150-km echoes over Jicamarca based on low-power VHF observationsVIPIR and 50 MHz Radar Studies of Gravity Wave Signatures in 150‐km Echoes Observed at JicamarcaThe Photoelectron‐Driven Upper Hybrid Instability as the Cause of 150‐km EchoesHeight Variation of Gaps in 150‐km Echoes and Whole Atmosphere Community Climate Model Electron Densities Suggest Link to Upper Hybrid ResonanceOn the Type‐A and Type‐B 150‐km Radar EchoesHigh resolution observations of 150 km echoes at JicamarcaSolar Flare Effects on 150‐km Echoes Observed Over Jicamarca: WACCM‐X SimulationsUnexpected characteristics of the 150 km echoes observed over Gadanki and their implicationsRadar observations of daytime 150‐km echoes from outside the equatorial electrojet belt over GadankiSq and EEJ—A Review on the Daily Variation of the Geomagnetic Field Caused by Ionospheric Dynamo CurrentsA comparative study of equatorial daytime vertical E × B drift in the Indian and Indonesian sectors based on 150 km echoesInteraction between direct penetration and disturbance dynamo electric fields in the storm‐time equatorial ionosphereEquatorial Atmosphere Radar (EAR): System description and first resultsDescending ion layer property in the Gadanki radar observations of 150 km echoes and its implication to the echoing phenomenonDaytime 150‐km echoes observed with the Equatorial Atmosphere Radar in Indonesia: First resultsEvidence of a stratified echoing region at 150 kilometers in the vicinity of the magnetic equator during daylight hoursZonal asymmetry of daytime 150-km echoes observed by Equatorial Atmosphere Radar in IndonesiaDiscovery of two distinct types of equatorial 150 km radar echoesOn a summer maximum in the occurrence frequency of 150 km (<i>F</i><sub>1</sub>) radar echoes over PohnpeiNaturally enhanced ion-line spectra around the equatorial 150-km regionPhotoelectron‐induced waves: A likely source of 150 km radar echoes and enhanced electron modesOn the characteristics of 150-km echoes observed in the Brazilian longitude sector by the 30 MHz São Luís radarInternational Geomagnetic Reference Field : the thirteenth generation
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
- 学術機関リポジトリデータベース雑誌記事索引データベースCrossref科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベースCrossref
- Bibliographic ID (NDL)
- 12685400