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CiNii Research
Universal Scaling Laws for Solar and Stellar Atmospheric Heating
- 資料種別
- 記事
- 著者
- Shin Toriumiほか
- 出版者
- American Astronomical Society
- 出版年
- 2022-03-01
- 資料形態
- デジタル
- 掲載誌名
- The Astrophysical Journal 927 2
- 掲載ページ
- p.179-
資料詳細
要約等:
- <jats:title>Abstract</jats:title> <jats:p>The Sun and Sun-like stars commonly host multimillion-kelvin coronae and 10,000 K chromospher...
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デジタル
- 資料種別
- 記事
- 著者標目
- 出版年月日等
- 2022-03-01
- 出版年(W3CDTF)
- 2022-03-01
- タイトル(掲載誌)
- The Astrophysical Journal
- 巻号年月日等(掲載誌)
- 927 2
- 掲載巻
- 927
- 掲載号
- 2
- 掲載ページ
- 179-
- 掲載年月日(W3CDTF)
- 2022-03-01
- ISSN(掲載誌)
- 0004637X
- 出版事項(掲載誌)
- American Astronomical Society
- 対象利用者
- 一般
- DOI
- 10.3847/1538-4357/ac5179
- 作成日(W3CDTF)
- 2022-03-15
- オンライン閲覧公開範囲
- インターネット公開
- 著作権情報
- http://creativecommons.org/licenses/by/4.0/https://iopscience.iop.org/info/page/text-and-data-mining
- 関連情報(URI)
- 参照
- Reconstructing the XUV Spectra of Active Sun-like Stars Using Solar Scaling Relations with Magnetic FluxUniversal Scaling Laws for Solar and Stellar Atmospheric Heating: Catalog of Power-law Index between Solar Activity Proxies and Various Spectral IrradiancesSun-as-a-star Analyses of Various Solar Active Events Using Hα Spectral Images Taken by SMART/SDDI
- 参照
- Sun-as-a-star Spectral Irradiance Observations of Transiting Active RegionsInvestigation of Coronal Properties of X-Ray Bright G-dwarf Stars Based on the Solar Surface Magnetic Field–Corona RelationshipThe Helioseismic and Magnetic Imager (HMI) Investigation for the Solar Dynamics Observatory (SDO)Chromospheric variations in main-sequence starsStellar coronal X-ray emission and surface magnetic fluxSoft X-Ray Pulsations in Solar FlaresMagnetic cycles at different ages of starsMagnetic fields of young solar twinsCoronal Heating in Active Regions as a Function of Global Magnetic VariablesIn the Trenches of the Solar–Stellar Connection. II. Extreme Ultraviolet Flux–Flux Correlations across Solar Cycle 2425 Years of Self-Organized Criticality: Solar and AstrophysicsSuperflares on solar-type starsSolar Flares: Magnetohydrodynamic ProcessesXUV Photometer System (XPS): Solar Variations during the SORCE MissionSpectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search ProgramsCorona and XUV emission modelling of the Sun and Sun-like starsEstimating Magnetic Filling Factors from Zeeman–Doppler MagnetogramsOn-Orbit Performance of the Helioseismic and Magnetic Imager Instrument onboard the Solar Dynamics ObservatoryX-ray studies of coeval star samples. III - X-ray emission in the Ursa Major streamDoppler imaging of LQ Hydrae for 1998–2002Solar–Stellar Irradiance Comparison Experiment II (Solstice II): Instrument Concept and DesignMAGNETIC PROPERTIES OF SOLAR ACTIVE REGIONS THAT GOVERN LARGE SOLAR FLARES AND ERUPTIONSFlare-productive active regionsEvolution of the Solar Activity over Time and Effects on Planetary Atmospheres. I. High‐Energy Irradiances (1–1700 A)Temporal evolution and correlations of optical activity indicators measured in Sun-as-a-star observationsHidden magnetic fields of young sunsLimits to the accuracy of the 10.7 cm fluxImprovements in the Determination of ISS Ca ii K ParametersOverview of the Solar Radiation and Climate Experiment (SORCE) Seventeen-Year MissionImpact of space weather on climate and habitability of terrestrial-type exoplanetsThe X‐Ray Sun in Time: A Study of the Long‐Term Evolution of Coronae of Solar‐Type StarsStructure and Evolution of Nearby Stars with Planets. II. Physical Properties of ∼1000 Cool Stars from the SPOCS CatalogOn the statistical description of inhomogeneities in the quiet solar atmosphere. I - Linear regression analysis and absolute calibration of multichannel observations of the Ca/+/ emission networkEmission of solar chromospheric and transition region features related to the underlying magnetic fieldCoronal temperature, density, and magnetic field maps of a solar acitve region using the Owens Valley Solar ArrayX-ray astronomy of stellar coronaeTHE FORMATION OF<i>IRIS</i>DIAGNOSTICS. II. THE FORMATION OF THE Mg II h&k LINES IN THE SOLAR ATMOSPHEREHEATING OF THE SOLAR CHROMOSPHERE AND CORONA BY ALFVÉN WAVE TURBULENCEAtmospheric Beacons of Life from Exoplanets Around G and K StarsParent stars of extrasolar planets - X. Lithium abundances and<i>v</i>sin <i>i</i>revisitedTime Scales for CA II Emission Decay, Rotational Braking, and Lithium DepletionSun‐as‐a‐Star Spectrum Variations 1974–2006RESOLVING THE ξ BOO BINARY WITH<i>CHANDRA</i>, AND REVEALING THE SPECTRAL TYPE DEPENDENCE OF THE CORONAL “FIP EFFECT”Host Stars and their Effects on Exoplanet AtmospheresAn Observational Overview of Solar FlaresMass and Energy Flow in the Solar Chromosphere and CoronaTopological Dissipation and the Small-Scale Fields in Turbulent GasesThe Solar Dynamics Observatory (SDO)Prebiotic chemistry and atmospheric warming of early Earth by an active young SunThe stellar activity-rotation relationship revisited: Dependence of saturated and non-saturated X-ray emission regimes on stellar mass for late-type dwarfsDesign and Ground Calibration of the Helioseismic and Magnetic Imager (HMI) Instrument on the Solar Dynamics Observatory (SDO)Stellar Lyα Emission Lines in the <i>Hubble Space Telescope</i> Archive: Intrinsic Line Fluxes and Absorption from the Heliosphere and AstrospheresCoronal Evolution of the Sun in Time: High‐Resolution X‐Ray Spectroscopy of Solar Analogs with Different AgesFormation of chromospheric lines in cool dwarf starsNanoflares and the solar X-ray coronaChromospheric variations in main-sequence starsEvaluating (and Improving) Estimates of the Solar Radial Magnetic Field Component from Line-of-Sight MagnetogramsTHE STELLAR-ACTIVITY-ROTATION RELATIONSHIP AND THE EVOLUTION OF STELLAR DYNAMOSEphemeral Regions on a Sequence of Full‐Disk Michelson Doppler Imager MagnetogramsThe Relationship Between X‐Ray Radiance and Magnetic FluxPower Laws in Solar Flares: Self-Organized Criticality or Turbulence?Stellar magnetism: empirical trends with age and rotationRelations between the photospheric magnetic field and the emission from the outer atmospheres of cool stars. I - The solar CA II K line core emissionTHE FORMATION OF THE Hα LINE IN THE SOLAR CHROMOSPHEREOn Solving the Coronal Heating ProblemFundamental parameters and infrared excesses of<i>Hipparcos</i>starsThe Spectral Irradiance Monitor: Scientific Requirements, Instrument Design, and Operation ModesPhysical Processes in Magnetically Driven Flares on the Sun, Stars, and Young Stellar ObjectsThe ROSAT missionOn the Generation, Propagation, and Reflection of Alfven Waves from the Solar Photosphere to the Distant HeliosphereThe 10.7 cm solar radio flux (<i>F</i><sub>10.7</sub>)THE KEPLER CATALOG OF STELLAR FLARESThe Sun in Time: Activity and EnvironmentThe relationship between chromospheric emissions and magnetic field strength
- 連携機関・データベース
- 国立情報学研究所 : CiNii Research
- 提供元機関・データベース
- Crossref科学研究費助成事業データベースCrossrefCrossrefCrossref