Validation of computed extreme ultraviolet emission spectra during solar flares
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DOI[10.1186/s40623-021-01402-7]to the data of the same series
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- Material Type
- 記事
- Author/Editor
- Shohei NishimotoKyoko WatanabeToshiki Kawai
- Publication, Distribution, etc.
- Publication Date
- 2021-03-25
- Publication Date (W3CDTF)
- 2021-03-25
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 73(79)
- Volume
- 73(79)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-021-01402-7
- Persistent ID (NDL)
- info:ndljp/pid/11667976
- 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)
- 2021-04-28T11:35:34+09:00
- Date Captured (W3CDTF)
- 2021-04-28
- 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/11667897
- 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.
- 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/s40623-021-01402-710.21203/rs.3.rs-52084/v2
- Access Restrictions
- インターネット公開
- Related Material (URI)
- Is Referenced By
- Statistical analysis for EUV dynamic spectra and their impact on the ionosphere during solar flaresSpecial issue "Solar-terrestrial environment prediction : toward the synergy of science and forecasting operation of space weather and space climate"PSTEP : project for solar–terrestrial environment prediction
- References
- Energy Release Rates along Hα Flare Ribbons and the Location of Hard X‐Ray SourcesPseudo–Two‐dimensional Hydrodynamic Modeling of Solar Flare LoopsHEATING AND DYNAMICS OF TWO FLARE LOOP SYSTEMS OBSERVED BY AIA AND EISThe Extreme Ultraviolet Sensor (EUVS) for GOES-R<title>GOES x-ray sensor and its use in predicting solar-terrestrial disturbances</title>EVIDENCE FOR HOT FAST FLOW ABOVE A SOLAR FLARE ARCADEObservation and numerical modeling of chromospheric evaporation during the impulsive phase of a solar flareIRIS, Hinode, SDO, and RHESSI Observations of a White Light Flare Produced Directly by Non-thermal ElectronsThe Direct Relation between the Duration of Magnetic Reconnection and the Evolution of GOES Light Curves in Solar FlaresThe Atmospheric Imaging Assembly (AIA) on the Solar Dynamics Observatory (SDO)Variability of thermosphere and ionosphere responses to solar flaresThe GOES-R EUVS model for EUV irradiance variabilityExtreme Ultraviolet Variability Experiment (EVE) on the Solar Dynamics Observatory (SDO): Overview of Science Objectives, Instrument Design, Data Products, and Model DevelopmentsHinode Flare CatalogueSELF-ORGANIZATION OF RECONNECTING PLASMAS TO MARGINAL COLLISIONALITY IN THE SOLAR CORONANowcast of an EUV dynamic spectrum during solar flaresModel of the High-Energy Phase of Solar FlaresVELOCITY CHARACTERISTICS OF EVAPORATED PLASMA USING<i>HINODE</i>/EUV IMAGING SPECTROMETERSUDDEN DISTURBANCES OF THE IONOSPHERECHIANTI—An Atomic Database for Emission Lines. XV. Version 9, Improvements for the X-Ray Satellite LinesNEW SOLAR EXTREME-ULTRAVIOLET IRRADIANCE OBSERVATIONS DURING FLARESSolar EUV Experiment (SEE): Mission overview and first resultsSatellite remote sensing of thermospheric O/N<sub>2</sub> and solar EUV: 1. TheoryFirst Solar EUV Irradiances Obtained from SOHO by the Celias/SemENTHALPY-BASED THERMAL EVOLUTION OF LOOPS. III. COMPARISON OF ZERO-DIMENSIONAL MODELSMagnetic reconnection in the corona and the loop prominence phenomenonA FLARE OBSERVED IN CORONAL, TRANSITION REGION, AND HELIUM I 10830 Å EMISSIONSTheoretical model of flares and prominencesThe Flare Irradiance Spectral Model‐Version 2 (FISM2)Center-to-Limb Variability of Hot Coronal EUV Emissions During Solar FlaresFlare Irradiance Spectral Model (FISM): Daily component algorithms and resultsCHIANTI - an atomic database for emission linesSelf‐Consistent Magnetohydrodynamic Modeling of a Coronal Mass Ejection, Coronal Dimming, and a Giant Cusp‐shaped Arcade FormationFlare Irradiance Spectral Model (FISM): Flare component algorithms and resultsSpectroscopic Observations of Current Sheet Formation and EvolutionA time dependent relation between EUV solar flare light-curves from lines with differing formation temperaturesA Two-dimensional Magnetohydrodynamic Simulation of Chromospheric Evaporation in a Solar Flare Based on a Magnetic Reconnection ModelEvolution of Conjugate Footpoints inside Flare Ribbons during a Great Two‐Ribbon Flare on 2001 April 10Highly Efficient Modeling of Dynamic Coronal LoopsObservations of 1000 km s −1 Doppler shifts in 107 K solar flare supra-arcade
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
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