AKATSUKI returns to Venus
Available in National Diet Library
Find on the publisher's website
NDL Digital Collections
Digital data available
Check on the publisher's website
DOI[10.1186/s40623-016-0457-6]to the data of the same series
Holdings of Libraries in Japan
This page shows libraries in Japan other than the National Diet Library that hold the material.
Please contact your local library for information on how to use materials or whether it is possible to request materials from the holding libraries.
other
CiNii Research
Search ServicePaperYou can check the holdings of institutions and databases with which CiNii Research is linked at the site of CiNii Research.CiNii Research
Search ServiceDigitalYou can check the holdings of institutions and databases with which CiNii Research is linked at the site of CiNii Research.
Bibliographic Record
You can check the details of this material, its authority (keywords that refer to materials on the same subject, author's name, etc.), etc.
- Material Type
- 記事
- Author/Editor
- Masato NakamuraTakeshi ImamuraNobuaki Ishii
- Publication, Distribution, etc.
- Publication Date
- 2016-05-06
- Publication Date (W3CDTF)
- 2016-05-06
- Periodical title
- EPS : Earth, Planets and Space
- No. or year of volume/issue
- 68(75)
- Volume
- 68(75)
- ISSN (Periodical Title)
- 1880-5981
- ISSN-L (Periodical Title)
- 1343-8832
- Text Language Code
- eng
- DOI
- 10.1186/s40623-016-0457-6
- Persistent ID (NDL)
- info:ndljp/pid/9976818
- 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)
- 2016-05-17T18:44:59+09:00
- Date Captured (W3CDTF)
- 2016-05-17
- 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/9963599
- 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
- Collection (particular)
- 国立国会図書館デジタルコレクション > デジタル化資料 > 雑誌
- 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
- Holding library
- 国立国会図書館
- Call No.
- Z19-383
- Periodical Title (Persistent ID (NDL))
- info:ndljp/pid/3421918
- Data Provider (Database)
- 国立国会図書館 : 国立国会図書館雑誌記事索引
- Bibliographic ID (NDL)
- 9976818
- Bibliographic Record Category (NDL)
- 632
- 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/s40623-016-0457-6
- Access Restrictions
- インターネット公開
- Related Material
- AKATSUKI returns to Venus
- Related Material (URI)
- Is Referenced By
- Planetary-scale streak structure reproduced in a Venus atmospheric simulationOverview of Akatsuki data products: definition of data levels, method and accuracy of geometric correctionHow waves and turbulence maintain the super-rotation of Venus' atmospherePerformance of Akatsuki/IR2 in Venus orbit: the first yearAbsolute calibration of brightness temperature of the Venus disk observed by the Longwave Infrared Camera onboard AkatsukiStationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard AkatsukiInitial performance of the radio occultation experiment in the Venus orbiter mission AkatsukiMean winds at the cloud top of Venus obtained from two-wavelength UV imaging by AkatsukiTopographical and Local Time Dependence of Large Stationary Gravity Waves Observed at the Cloud Top of VenusGround-based observation of the cyclic nature and temporal variability of planetary-scale UV features at the Venus cloud top levelEquatorial jet in the lower to middle cloud layer of Venus revealed by AkatsukiPlanetary‐Scale Variations in Winds and UV Brightness at the Venusian Cloud Top: Periodicity and Temporal EvolutionVertical Coupling Between the Cloud‐Level Atmosphere and the Thermosphere of Venus Inferred From the Simultaneous Observations by Hisaki and AkatsukiThermal Tides in the Upper Cloud Layer of Venus as Deduced From the Emission Angle Dependence of the Brightness Temperature by Akatsuki/LIRCharacterising atmospheric gravity waves on the nightside lower clouds of Venus: a systematic analysisGigantic Vortices From Barotropic Instability Observed in the Atmosphere of VenusPeriodic Variation of Mesoscale Ultraviolet Contrast at the Cloud Top of VenusA GCM study of synoptic-scale vortices in the lower cloud layer on VenusProbing solar wind velocity from simultaneous superior solar conjunction radio science experiments of BepiColombo and Akatsuki missionsFine Vertical Structures at the Cloud Heights of Venus Revealed by Radio Holographic Analysis of Venus Express and Akatsuki Radio Occultation DataLarge stationary gravity wave in the atmosphere of VenusSuperrotation in Planetary AtmospheresHorizontal structures of bow-shaped mountain wave trains seen in thermal infrared images of venusian clouds taken by Akatsuki LIRGravity Wave Packets in the Venusian Atmosphere Observed by Radio Occultation Experiments: Comparison With Saturation TheoryBepiColombo Science Investigations During Cruise and Flybys at the Earth, Venus and MercuryKelvin Wave and Its Impact on the Venus Atmosphere Tested by Observing System Simulation ExperimentLong‐Term Variation of the Quasi‐Five‐Day Wave in the Top Layer of Venus CloudsIn-orbit recalibration of Longwave Infrared Camera onboard AkatsukiModeling a point-spread function originating from multiple reflection of light in the substrate of array sensor: the case of Akatsuki/IR2Dawn-dusk difference of periodic oxygen EUV dayglow variations at Venus observed by HisakiDynamical relationship between wind speed magnitude and meridional temperature contrast: Application to an interannual oscillation in Venusian middle atmosphere GCMLocal Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM ResultsStationary waves and slowly moving features in the night upper clouds of VenusNew cloud morphologies discovered on the Venus's night during AkatsukiA Long‐Lived Sharp Disruption on the Lower Clouds of VenusBrightness modulations of our nearest terrestrial planet Venus reveal atmospheric super-rotation rather than surface featuresInstrumental requirements for the study of Venus’ cloud top using the UV imaging spectrometer VeSUVThree‐Dimensional Structures of Thermal Tides Simulated by a Venus GCMScattering Properties of the Venusian Clouds Observed by the UV Imager on board AkatsukiVenus night-side photometry with “cleaned” Akatsuki/IR2 data: Aerosol properties and variations of carbon monoxideInvestigation of UV Absorbers on Venus Using the 283 and 365 nm Phase Curves Obtained From AkatsukiThe 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 DiscontinuityTwelve-Year Cycle in the Cloud Top Winds Derived from VMC/Venus Express and UVI/Akatsuki ImagingReflectivity of Venus’s Dayside Disk During the 2020 Observation Campaign: Outcomes and Future PerspectivesVenus cloud discontinuity in 2022The first assimilation of Akatsuki single-layer winds and its validation with Venusian atmospheric waves excited by solar heatingFormation of the Y Feature at the Venusian Cloud Top by Planetary‐Scale Waves and the Mean Circulation: Analysis of Venus Express VMC ImagesConstraints on Venus Lightning From Akatsuki's First 3 Years in OrbitPrincipal components of short-term variability in the ultraviolet albedo of VenusSolar-locked and geographical atmospheric structures inferred from a Venus general circulation model with radiative transferThermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultationLong-term Variations of Venus’s 365 nm Albedo Observed by Venus Express, Akatsuki, MESSENGER, and the Hubble Space Telescope小型月着陸実証機(SLIM)推進系の開発と運用Initial products of Akatsuki 1-μm cameraDevelopment and in-flight calibration of IR2 : 2-μm camera onboard Japan's Venus orbiter, AkatsukiVenus looks different from day to night across wavelengths : morphology from Akatsuki multispectral imagesUltraviolet imager on Venus orbiter Akatsuki and its initial resultsSpecial issue “Akatsuki at Venus : the first year of scientific operation”
- References
- Characteristic features in Venus’ nightside cloud-top temperature obtained by Akatsuki/LIRVenus's major cloud feature as an equatorially trapped wave distorted by the windFelsic highland crust on Venus suggested by Galileo Near‐Infrared Mapping Spectrometer dataOn observing the compositional variability of the surface of Venus using nightside near‐infrared thermal radiationMorphology of the cloud tops as observed by the Venus Express Monitoring CameraReturn to Venus of the Japanese Venus Climate Orbiter AKATSUKICloud top structure of Venus revealed by Subaru/COMICS mid-infrared imagesVenus’ clouds as inferred from the phase curves acquired by IR1 and IR2 on board AkatsukiVenus Express—The first European mission to VenusImages from Galileo of the Venus Cloud DeckPlanet-C: Venus Climate Orbiter mission of JapanHDO and SO<sub>2</sub>thermal mapping on VenusElucidating the Rate of Volcanism on Venus: Detection of Lava Eruptions Using Near-Infrared ObservationsA reanalysis of Venus winds at two cloud levels from Galileo SSI imagesLightning Detection by LAC Onboard the Japanese Venus Climate Orbiter, Planet-CStructure and meteorology of the middle atmosphere of Venus: Infrared remote sensing from the Pioneer OrbiterAutomated cloud tracking system for the Akatsuki Venus Climate Orbiter dataLong‐term variation in the cloud‐tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC imagesImproved automatic estimation of winds at the cloud top of Venus using superposition of cross-correlation surfacesLong-term variations of the UV contrast on Venus observed by the Venus Monitoring Camera on board Venus ExpressThe abundance and vertical distribution of the unknown ultraviolet absorber in the venusian atmosphere from analysis of Venus Monitoring Camera imagesUV contrasts and microphysical properties of the upper clouds of Venus from the UV and NIR VMC/VEx imagesLongwave Infrared Camera onboard the Venus Climate OrbiterHorizontal structure of planetary-scale waves at the cloud top of Venus deduced from Galileo SSI images with an improved cloud-tracking techniqueVariable winds on Venus mapped in three dimensionsVenus Monitoring Camera for Venus ExpressStructure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus ExpressThe atmosphere of VenusDetection of Sub-Micron Radiation from the Surface of Venus by Cassini/VIMSOverview of Venus orbiter, AkatsukiContrast sources for the infrared images taken by the Venus mission AkatsukiRadio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter AkatsukiScience 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)
- 雑誌記事索引データベースCrossref科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース科学研究費助成事業データベース学術機関リポジトリデータベースCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossrefCrossref
- Bibliographic ID (NDL)
- 9976818