Venus looks different from day to night across wavelengths : morphology from Akatsuki multispectral images
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DOI[10.1186/s40623-018-0789-5]のデータに遷移します
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- 資料種別
- 記事
- 著者・編者
- Sanjay S. LimayeShigeto WatanabeAtsushi Yamazaki
- 出版年月日等
- 2018-02-12
- 出版年（W3CDTF）
- 2018-02-12
- タイトル（掲載誌）
- EPS : Earth, Planets and Space
- 巻号年月日等（掲載誌）
- 70(24)
- 掲載巻
- 70(24)
- 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/s40623-018-0789-5
- 国立国会図書館永続的識別子
- info:ndljp/pid/11067480
- コレクション（共通）
- コレクション（障害者向け資料：レベル1）
- 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
- 収集根拠
- オンライン資料収集制度
- 受理日（W3CDTF）
- 2018-04-12T16:47:48+09:00
- 保存日（W3CDTF）
- 2018-04-12
- 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（国立国会図書館永続的識別子）
- info:ndljp/pid/11067456
- 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
- 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/s40623-018-0789-5
- 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）
- 参照
- A GCM study of synoptic-scale vortices in the lower cloud layer on VenusFormation and Quasi‐Periodic Variation of Equatorial Jet Caused by Planetary‐Scale Waves in the Venusian Lower Cloud LayerVenus cloud discontinuity in 2022Vertical‐Wind‐Induced Cloud Opacity Variation in Low Latitudes Simulated by a Venus GCMGigantic Vortices From Barotropic Instability Observed in the Atmosphere of VenusCorrelation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various WavelengthsIn situ biochemical characterization of Venus cloud particles using a life-signature detection microscopeA GCM Study on the 4‐Day and 5‐Day Waves in the Venus AtmosphereAmateur Observers Witness the Return of Venus’ Cloud DiscontinuityPlanetary‐Scale Waves Seen in Thermal Infrared Images of Venusian Cloud TopThe nightside cloud-top circulation of the atmosphere of VenusVenus night-side photometry with “cleaned” Akatsuki/IR2 data: Aerosol properties and variations of carbon monoxideA Long‐Lived Sharp Disruption on the Lower Clouds of VenusNew cloud morphologies discovered on the Venus's night during AkatsukiStationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard AkatsukiMorphology and Dynamics of Venus's Middle Clouds With Akatsuki/IR1Planetary-scale streak structure reproduced in a Venus atmospheric simulationNightside Winds at the Lower Clouds of Venus with Akatsuki/IR2: Longitudinal, Local Time, and Decadal Variations from Comparison with Previous MeasurementsSpecial issue “Akatsuki at Venus : the first year of scientific operation”Ultraviolet imager on Venus orbiter Akatsuki and its initial results
- 参照
- Initial products of Akatsuki 1-μm cameraPerformance of Akatsuki/IR2 in Venus orbit: the first yearAbsolute calibration of brightness temperature of the Venus disk observed by the Longwave Infrared Camera onboard AkatsukiMorphology and temporal variation of the polar oval of Venus revealed by VMC/Venus express visible and UV imagesRetrieval of Venus' cloud parameters from VIRTIS nightside spectra in the latitude band 25°-55°NVenus Climate Orbiter Akatsuki IR2 Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki LIR Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki IR1 Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki UVI Calibrated Data PDS3 datasetScattering Properties of the Venusian Clouds Observed by the UV Imager on board AkatsukiVenus's winds and temperatures during the MESSENGER's flyby: An approximation to a three‐dimensional instantaneous state of the atmosphereOn the iron chloride aerosol in the clouds of VenusRadiative energy balance of Venus: An approach to parameterize thermal cooling and solar heating ratesLarge stationary gravity wave in the atmosphere of VenusHDO and SO<sub>2</sub>thermal mapping on VenusAerosol properties in the upper haze of Venus from SPICAV IR dataSensitivity of net thermal flux to the abundance of trace gases in the lower atmosphere of VenusSulfur aerosol in the clouds of VenusAKATSUKI returns to VenusDevelopment and in-flight calibration of IR2 : 2-μm camera onboard Japan's Venus orbiter, AkatsukiThe VMC/VEx photometry at small phase angles: Glory and the physical properties of particles in the upper cloud layer of VenusSix years of Venus winds at the upper cloud level from UV, visible and near infrared observations from VIRTIS on Venus ExpressVenus's major cloud feature as an equatorially trapped wave distorted by the windInstantaneous three-dimensional thermal structure of the South Polar Vortex of VenusCloud top structure of Venus revealed by Subaru/COMICS mid-infrared imagesGlory on Venus cloud tops and the unknown UV absorberHigh latitude gravity waves at the Venus cloud tops as observed by the Venus Monitoring Camera on board Venus ExpressHDO and SO<sub>2</sub>thermal mapping on VenusA chaotic long-lived vortex at the southern pole of VenusModels of the global cloud structure on Venus derived from Venus Express observationsAssessing the long-term variability of Venus winds at cloud level from VIRTIS–Venus ExpressMorphology of the cloud tops as observed by the Venus Express Monitoring CameraScience requirements and description of the 1 μm camera onboard the Akatsuki Venus OrbiterDynamics and circulation regimes of terrestrial planetsVenus’s Southern Polar Vortex Reveals Precessing CirculationOverview of Venus orbiter, AkatsukiLIR : Longwave Infrared Camera onboard the Venus orbiter AkatsukiContrast sources for the infrared images taken by the Venus mission AkatsukiAn investigation of the SO2 content of the venusian mesosphere using SPICAV-UV in nadir modePhotolysis of sulphuric acid as the source of sulphur oxides in the mesosphere of VenusIn-flight performance of MESSENGER's Mercury Dual Imaging SystemAltimetry of the Venus cloud tops from the Venus Express observationsAnalysis of thermal emission from the nightside of Venus at 1.51 and 1.55 μmVariability of CO concentrations in the Venus troposphere from Venus Express/VIRTIS using a Band Ratio TechniqueVortex circulation on Venus: Dynamical similarities with terrestrial hurricanesAtmospheric structure and dynamics as the cause of ultraviolet markings in the clouds of VenusEvidence for anomalous cloud particles at the poles of VenusVariable winds on Venus mapped in three dimensionsLightning Detection by LAC Onboard the Japanese Venus Climate Orbiter, Planet-CCharacterization of mesoscale gravity waves in the upper and lower clouds of Venus from VEX‐VIRTIS imagesSouth-polar features on Venus similar to those near the north poleChemical kinetic model for the lower atmosphere of VenusVenus Monitoring Camera for Venus ExpressA review of selected issues concerning the chemistry in Venus’ middle atmosphereScientific goals for the observation of Venus by VIRTIS on ESA/Venus express missionA reanalysis of Venus winds at two cloud levels from Galileo SSI imagesVenus Express—The first European mission to VenusLongwave Infrared Camera onboard the Venus Climate OrbiterAtmospheric composition, chemistry, and cloudsSaturn's Temperature Field from High-Resolution Middle-Infrared ImagingMicroorganisms cultured from stratospheric air samples obtained at 41 kmGlobal-Scale Winds at the Venus Cloud-Top Inferred from Cloud Streak Orientationsセミスペクトルモデルを用いた回転水槽中の流れパターンの遷移に関する数値的研究Galileo Infrared Imaging Spectroscopy Measurements at VenusImages from Galileo of the Venus Cloud DeckThermal Maps of Jupiter: Spatial Organization and Time Dependence of Stratospheric Temperatures, 1980 to 1990Characteristics of Gravity Waves Generated by Surface Topography on Venus: Comparison with the VEGA Balloon ResultsImplications of the VEGA Balloon Results for Venus Atmospheric DynamicsVenus atmospheric circulation: Observations and implications of the thermal structurePrefaceMorphology and movements of polarizations features on Venus as seen in the pioneer Orbiter Cloud Photopolarimeter dataCloud structure on the dark side of VenusUltraviolet contrasts and the absorbers near the Venus cloud topsStructure and meteorology of the middle atmosphere of Venus: Infrared remote sensing from the Pioneer OrbiterThe clouds of Venus: A synthesis reportCloud morphology and motions from Pioneer Venus imagesThe character of the thermal emission from VenusThe microphysics of the clouds of Venus: Results of the Pioneer Venus Particle Size Spectrometer ExperimentCloud and haze properties from Pioneer Venus polarimetryClouds of Venus: A Preliminary Assessment of MicrostructureOrbiter Cloud Photopolarimeter InvestigationVenus: Further Evidence of Vortex CirculationVenus exploration with the Venera 9 and Venera 10 spacecraftOn the Origin of Ultraviolet Contrasts on VenusVenus: Evolution of the Upper Atmospheric CloudsInterpretation of the Polarization of VenusVenus: Atmospheric Motion and Structure from Mariner 10 PicturesAre the clouds of venus sulfuric acid?Venus Cloud ContrastsSome experiments on thermal convection in a rotating liquidThe reciprocity principle in lunar photometryPhotographs of VenusTHE CLOUDS OF VENUS AND THEIR SIGNIFICANCE.<sup>1</sup>
- 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
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