Venus looks different from day to night across wavelengths : morphology from Akatsuki multispectral images
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- Material Type
- 記事
- Author/Editor
- Sanjay S. LimayeShigeto WatanabeAtsushi Yamazaki
- Publication, Distribution, etc.
- Publication Date
- 2018-02-12
- Publication Date (W3CDTF)
- 2018-02-12
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 70(24)
- Volume
- 70(24)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-018-0789-5
- Persistent ID (NDL)
- info:ndljp/pid/11067480
- 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)
- 2018-04-12T16:47:48+09:00
- Date Captured (W3CDTF)
- 2018-04-12
- 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/11067456
- 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/s40623-018-0789-5
- Access Restrictions
- インターネット公開
- Related Material (URI)
- Is Referenced By
- Planetary-scale streak structure reproduced in a Venus atmospheric simulationStationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard AkatsukiGigantic Vortices From Barotropic Instability Observed in the Atmosphere of VenusIn situ biochemical characterization of Venus cloud particles using a life-signature detection microscopeA GCM study of synoptic-scale vortices in the lower cloud layer on VenusMorphology and Dynamics of Venus's Middle Clouds With Akatsuki/IR1Planetary‐Scale Waves Seen in Thermal Infrared Images of Venusian Cloud TopFormation and Quasi‐Periodic Variation of Equatorial Jet Caused by Planetary‐Scale Waves in the Venusian Lower Cloud LayerNightside Winds at the Lower Clouds of Venus with Akatsuki/IR2: Longitudinal, Local Time, and Decadal Variations from Comparison with Previous MeasurementsNew cloud morphologies discovered on the Venus's night during AkatsukiA Long‐Lived Sharp Disruption on the Lower Clouds of VenusA GCM Study on the 4‐Day and 5‐Day Waves in the Venus AtmosphereVenus night-side photometry with “cleaned” Akatsuki/IR2 data: Aerosol properties and variations of carbon monoxideThe nightside cloud-top circulation of the atmosphere of VenusCorrelation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various WavelengthsAmateur Observers Witness the Return of Venus’ Cloud DiscontinuityVenus cloud discontinuity in 2022Vertical‐Wind‐Induced Cloud Opacity Variation in Low Latitudes Simulated by a Venus GCMUltraviolet imager on Venus orbiter Akatsuki and its initial resultsSpecial issue “Akatsuki at Venus : the first year of scientific operation”
- References
- Performance of Akatsuki/IR2 in Venus orbit: the first yearAbsolute calibration of brightness temperature of the Venus disk observed by the Longwave Infrared Camera onboard AkatsukiSensitivity of net thermal flux to the abundance of trace gases in the lower atmosphere of VenusHDO and SO<sub>2</sub>thermal mapping on VenusChemical kinetic model for the lower atmosphere of VenusVariability of CO concentrations in the Venus troposphere from Venus Express/VIRTIS using a Band Ratio TechniqueCloud and haze properties from Pioneer Venus polarimetryPhotolysis of sulphuric acid as the source of sulphur oxides in the mesosphere of VenusA chaotic long-lived vortex at the southern pole of VenusPrefaceVenus's major cloud feature as an equatorially trapped wave distorted by the windThe microphysics of the clouds of Venus: Results of the Pioneer Venus Particle Size Spectrometer ExperimentSaturn's Temperature Field from High-Resolution Middle-Infrared ImagingThe character of the thermal emission from VenusOn the iron chloride aerosol in the clouds of VenusTHE CLOUDS OF VENUS AND THEIR SIGNIFICANCE.<sup>1</sup>Dynamics and circulation regimes of terrestrial planetsMorphology of the cloud tops as observed by the Venus Express Monitoring CameraVenus: Evolution of the Upper Atmospheric CloudsCloud top structure of Venus revealed by Subaru/COMICS mid-infrared imagesLarge stationary gravity wave in the atmosphere of VenusVenus Express—The first European mission to VenusThe reciprocity principle in lunar photometryGlobal-Scale Winds at the Venus Cloud-Top Inferred from Cloud Streak OrientationsCloud morphology and motions from Pioneer Venus imagesImages from Galileo of the Venus Cloud DeckVortex circulation on Venus: Dynamical similarities with terrestrial hurricanesCharacterization of mesoscale gravity waves in the upper and lower clouds of Venus from VEX‐VIRTIS imagesCharacteristics of Gravity Waves Generated by Surface Topography on Venus: Comparison with the VEGA Balloon ResultsAtmospheric composition, chemistry, and cloudsIn-flight performance of MESSENGER's Mercury Dual Imaging SystemHDO and SO<sub>2</sub>thermal mapping on VenusInstantaneous three-dimensional thermal structure of the South Polar Vortex of VenusVenus's winds and temperatures during the MESSENGER's flyby: An approximation to a three‐dimensional instantaneous state of the atmosphereSome experiments on thermal convection in a rotating liquidEvidence for anomalous cloud particles at the poles of VenusVenus: Atmospheric Motion and Structure from Mariner 10 PicturesA reanalysis of Venus winds at two cloud levels from Galileo SSI imagesThe clouds of Venus: A synthesis reportLightning Detection by LAC Onboard the Japanese Venus Climate Orbiter, Planet-CInterpretation of the Polarization of VenusVenus exploration with the Venera 9 and Venera 10 spacecraftStructure and meteorology of the middle atmosphere of Venus: Infrared remote sensing from the Pioneer OrbiterAssessing the long-term variability of Venus winds at cloud level from VIRTIS–Venus ExpressSulfur aerosol in the clouds of VenusAtmospheric structure and dynamics as the cause of ultraviolet markings in the clouds of VenusOn the Origin of Ultraviolet Contrasts on VenusAre the clouds of venus sulfuric acid?Scientific goals for the observation of Venus by VIRTIS on ESA/Venus express missionSouth-polar features on Venus similar to those near the north poleVenus’s Southern Polar Vortex Reveals Precessing CirculationAnalysis of thermal emission from the nightside of Venus at 1.51 and 1.55 μmClouds of Venus: A Preliminary Assessment of MicrostructureA review of selected issues concerning the chemistry in Venus’ middle atmosphereAerosol properties in the upper haze of Venus from SPICAV IR dataUltraviolet contrasts and the absorbers near the Venus cloud topsOrbiter Cloud Photopolarimeter InvestigationCloud structure on the dark side of VenusMicroorganisms cultured from stratospheric air samples obtained at 41 kmMorphology and temporal variation of the polar oval of Venus revealed by VMC/Venus express visible and UV imagesLongwave Infrared Camera onboard the Venus Climate OrbiterScattering Properties of the Venusian Clouds Observed by the UV Imager on board AkatsukiSix years of Venus winds at the upper cloud level from UV, visible and near infrared observations from VIRTIS on Venus ExpressImplications of the VEGA Balloon Results for Venus Atmospheric DynamicsThermal Maps of Jupiter: Spatial Organization and Time Dependence of Stratospheric Temperatures, 1980 to 1990Venus Cloud ContrastsGalileo Infrared Imaging Spectroscopy Measurements at VenusAn investigation of the SO2 content of the venusian mesosphere using SPICAV-UV in nadir modeMorphology and movements of polarizations features on Venus as seen in the pioneer Orbiter Cloud Photopolarimeter dataHigh latitude gravity waves at the Venus cloud tops as observed by the Venus Monitoring Camera on board Venus ExpressRadiative energy balance of Venus: An approach to parameterize thermal cooling and solar heating ratesVariable winds on Venus mapped in three dimensionsAltimetry of the Venus cloud tops from the Venus Express observationsVenus Monitoring Camera for Venus ExpressModels of the global cloud structure on Venus derived from Venus Express observationsThe VMC/VEx photometry at small phase angles: Glory and the physical properties of particles in the upper cloud layer of VenusPhotographs of VenusVenus: Further Evidence of Vortex CirculationVenus atmospheric circulation: Observations and implications of the thermal structureGlory on Venus cloud tops and the unknown UV absorberRetrieval of Venus' cloud parameters from VIRTIS nightside spectra in the latitude band 25°-55°N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Venus Climate Orbiter Akatsuki UVI Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki IR1 Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki LIR Calibrated Data PDS3 datasetVenus Climate Orbiter Akatsuki IR2 Calibrated Data PDS3 datasetOverview of Venus orbiter, AkatsukiInitial products of Akatsuki 1-μm cameraDevelopment and in-flight calibration of IR2 : 2-μm camera onboard Japan's Venus orbiter, AkatsukiContrast sources for the infrared images taken by the Venus mission AkatsukiAKATSUKI returns to VenusScience requirements and description of the 1 μm camera onboard the Akatsuki Venus OrbiterLIR : Longwave Infrared Camera onboard the Venus orbiter Akatsuki
- Data Provider (Database)
- 国立情報学研究所 : CiNii Research
- Original Data Provider (Database)
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