Validation of computed extreme ultraviolet emission spectra during solar flares

• 資料種別: 記事
• タイトル: Validation of computed extreme ultraviolet emission spectra during solar flares
• 著者・編者: Shohei Nishimoto; Kyoko Watanabe; Toshiki Kawai
• 出版事項: 日本 : Springer Nature
• 出版年月日等: 2021-03-25
• 出版年（W3CDTF）: 2021-03-25
• タイトル（掲載誌）: EPS : Earth, Planets and Space
• 巻号年月日等（掲載誌）: 73(79)
• 掲載巻: 73(79)
• ISSN（掲載誌）: 1880-5981
• ISSN-L（掲載誌）: 1343-8832
• 本文の言語コード: eng
• DOI: 10.1186/s40623-021-01402-7; https://doi.org/10.1186/s40623-021-01402-7
• 国立国会図書館永続的識別子: info:ndljp/pid/11667976; https://dl.ndl.go.jp/pid/11667976
• コレクション（共通）: 障害者向け資料
• コレクション（障害者向け資料：レベル1）: テキストデータ
• コレクション（個別）: 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; https://dl.ndl.go.jp/collections/B00035
• 収集根拠: オンライン資料収集制度
• 受理日（W3CDTF）: 2021-04-28T11:35:34+09:00
• 保存日（W3CDTF）: 2021-04-28
• 記録形式（IMT）: application/pdf
• オンライン閲覧公開範囲: 国立国会図書館内限定公開
• デジタル化資料送信: 図書館・個人送信対象外
• 遠隔複写可否（NDL）: 可
• 掲載誌（URI）: https://earth-planets-space.springeropen.com/articles
• 掲載誌（国立国会図書館永続的識別子）: info:ndljp/pid/11667897; https://dl.ndl.go.jp/pid/11667897
• 連携機関・データベース: 国立国会図書館 : 国立国会図書館デジタルコレクション; https://dl.ndl.go.jp

• 要約等: コレクション : 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
• DOI: 10.1186/s40623-021-01402-7; https://doi.org/10.1186/s40623-021-01402-7; 10.21203/rs.3.rs-52084/v2; https://doi.org/10.21203/rs.3.rs-52084/v2
• オンライン閲覧公開範囲: インターネット公開
• 関連情報（URI）: http://id.ndl.go.jp/digimeta/11667976; https://dl.ndl.go.jp/pid/11667976; http://link.springer.com/content/pdf/10.1186/s40623-021-01402-7.pdf; http://link.springer.com/article/10.1186/s40623-021-01402-7/fulltext.html; https://www.researchsquare.com/article/rs-52084/v2; https://www.researchsquare.com/article/rs-52084/v2.html
• 参照: Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flares; https://cir.nii.ac.jp/crid/1360580229817817600; Special issue "Solar-terrestrial environment prediction : toward the synergy of science and forecasting operation of space weather and space climate"; https://cir.nii.ac.jp/crid/2050307417129948032; PSTEP : project for solar–terrestrial environment prediction; https://cir.nii.ac.jp/crid/2050588892104455680
• 参照: Energy Release Rates along Hα Flare Ribbons and the Location of Hard X‐Ray Sources; https://cir.nii.ac.jp/crid/1360011143688186880; Pseudo–Two‐dimensional Hydrodynamic Modeling of Solar Flare Loops; https://cir.nii.ac.jp/crid/1360011144221207552; HEATING AND DYNAMICS OF TWO FLARE LOOP SYSTEMS OBSERVED BY AIA AND EIS; https://cir.nii.ac.jp/crid/1360011144670120832; The Extreme Ultraviolet Sensor (EUVS) for GOES-R; https://cir.nii.ac.jp/crid/1360011145043521408; <title>GOES x-ray sensor and its use in predicting solar-terrestrial disturbances</title>; https://cir.nii.ac.jp/crid/1360011146558348288; EVIDENCE FOR HOT FAST FLOW ABOVE A SOLAR FLARE ARCADE; https://cir.nii.ac.jp/crid/1360283692449006208; Observation and numerical modeling of chromospheric evaporation during the impulsive phase of a solar flare; https://cir.nii.ac.jp/crid/1360285708892265088; IRIS, Hinode, SDO, and RHESSI Observations of a White Light Flare Produced Directly by Non-thermal Electrons; https://cir.nii.ac.jp/crid/1360285714649950592; The Direct Relation between the Duration of Magnetic Reconnection and the Evolution of GOES Light Curves in Solar Flares; https://cir.nii.ac.jp/crid/1360285714651188608; The Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO); https://cir.nii.ac.jp/crid/1360292617917560448; Variability of thermosphere and ionosphere responses to solar flares; https://cir.nii.ac.jp/crid/1360292618472375552; The GOES-R EUVS model for EUV irradiance variability; https://cir.nii.ac.jp/crid/1360292618582266496; Extreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model Developments; https://cir.nii.ac.jp/crid/1360292619317244928; Hinode Flare Catalogue; https://cir.nii.ac.jp/crid/1360565165385260032; SELF-ORGANIZATION OF RECONNECTING PLASMAS TO MARGINAL COLLISIONALITY IN THE SOLAR CORONA; https://cir.nii.ac.jp/crid/1360848659311839232; Nowcast of an EUV dynamic spectrum during solar flares; https://cir.nii.ac.jp/crid/1360849941905408128; Model of the High-Energy Phase of Solar Flares; https://cir.nii.ac.jp/crid/1360855569580171776; VELOCITY CHARACTERISTICS OF EVAPORATED PLASMA USING<i>HINODE</i>/EUV IMAGING SPECTROMETER; https://cir.nii.ac.jp/crid/1360855570062166528; SUDDEN DISTURBANCES OF THE IONOSPHERE; https://cir.nii.ac.jp/crid/1360855570820922240; CHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite Lines; https://cir.nii.ac.jp/crid/1361137045479513728; NEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARES; https://cir.nii.ac.jp/crid/1361418520015956480; Solar EUV Experiment (SEE): Mission overview and first results; https://cir.nii.ac.jp/crid/1361699993398289664; Satellite remote sensing of thermospheric O/N₂ and solar EUV: 1. Theory; https://cir.nii.ac.jp/crid/1361699994792310912; First Solar EUV Irradiances Obtained from SOHO by the Celias/Sem; https://cir.nii.ac.jp/crid/1362262943507396608; ENTHALPY-BASED THERMAL EVOLUTION OF LOOPS. III. COMPARISON OF ZERO-DIMENSIONAL MODELS; https://cir.nii.ac.jp/crid/1362262943898035712; Magnetic reconnection in the corona and the loop prominence phenomenon; https://cir.nii.ac.jp/crid/1362544420949853184; A FLARE OBSERVED IN CORONAL, TRANSITION REGION, AND HELIUM I 10830 Å EMISSIONS; https://cir.nii.ac.jp/crid/1362825895035375744; Theoretical model of flares and prominences; https://cir.nii.ac.jp/crid/1363107368245568512; The Flare Irradiance Spectral Model‐Version 2 (FISM2); https://cir.nii.ac.jp/crid/1363107369992903168; Center-to-Limb Variability of Hot Coronal EUV Emissions During Solar Flares; https://cir.nii.ac.jp/crid/1363107370479923328; Flare Irradiance Spectral Model (FISM): Daily component algorithms and results; https://cir.nii.ac.jp/crid/1363388844226139008; CHIANTI - an atomic database for emission lines; https://cir.nii.ac.jp/crid/1363388845816309376; Self‐Consistent Magnetohydrodynamic Modeling of a Coronal Mass Ejection, Coronal Dimming, and a Giant Cusp‐shaped Arcade Formation; https://cir.nii.ac.jp/crid/1363388845874410496; Flare Irradiance Spectral Model (FISM): Flare component algorithms and results; https://cir.nii.ac.jp/crid/1363388846134410624; Spectroscopic Observations of Current Sheet Formation and Evolution; https://cir.nii.ac.jp/crid/1363388846221200128; A time dependent relation between EUV solar flare light-curves from lines with differing formation temperatures; https://cir.nii.ac.jp/crid/1363670319017957632; A Two-dimensional Magnetohydrodynamic Simulation of Chromospheric Evaporation in a Solar Flare Based on a Magnetic Reconnection Model; https://cir.nii.ac.jp/crid/1363670319344438016; Evolution of Conjugate Footpoints inside Flare Ribbons during a Great Two‐Ribbon Flare on 2001 April 10; https://cir.nii.ac.jp/crid/1363670320087381888; Highly Efficient Modeling of Dynamic Coronal Loops; https://cir.nii.ac.jp/crid/1363670321243638144; Observations of 1000 km s −1 Doppler shifts in 107 K solar flare supra-arcade; https://cir.nii.ac.jp/crid/1364233270287548032
• 連携機関・データベース: 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• 提供元機関・データベース: 雑誌記事索引データベース; https://ndlsearch.ndl.go.jp; Crossref; https://www.crossref.org; 科学研究費助成事業データベース; https://kaken.nii.ac.jp/ja
• 書誌ID（NDLBibID）: 11667976; http://id.ndl.go.jp/bib/11667976