Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki

• 資料種別: 記事
• タイトル: Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki
• 著者・編者: Takeshi Imamura; Hiroki Ando; Silvia Tellmann
• 出版事項: 日本 : Springer Nature
• 出版年月日等: 2017-10-03
• 出版年（W3CDTF）: 2017-10-03
• タイトル（掲載誌）: EPS : Earth, Planets and Space
• 巻号年月日等（掲載誌）: 69(137)
• 掲載巻: 69(137)
• 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/s40623-017-0722-3; https://doi.org/10.1186/s40623-017-0722-3
• 国立国会図書館永続的識別子: info:ndljp/pid/11002663; https://dl.ndl.go.jp/pid/11002663
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• コレクション（障害者向け資料：レベル1）: テキストデータ
• 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; https://dl.ndl.go.jp/collections/B00035
• 収集根拠: オンライン資料収集制度
• 受理日（W3CDTF）: 2017-12-14T17:18:17+09:00
• 保存日（W3CDTF）: 2017-12-12
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• 掲載誌（URI）: https://earth-planets-space.springeropen.com/articles?searchType=journalSearch&sort=PubDate&page=2
• 掲載誌（国立国会図書館永続的識別子）: info:ndljp/pid/10319651; https://dl.ndl.go.jp/pid/10319651
• 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; https://dl.ndl.go.jp

• 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/s40623-017-0722-3; https://doi.org/10.1186/s40623-017-0722-3
• 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: © The Author(s) 2017.; This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
• 関連情報: Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki; https://cir.nii.ac.jp/crid/2120026414383223680
• 関連情報（URI）: https://hdl.handle.net/20.500.14094/90004975; http://id.ndl.go.jp/digimeta/11002663; https://dl.ndl.go.jp/pid/11002663; http://link.springer.com/content/pdf/10.1186/s40623-017-0722-3.pdf; http://link.springer.com/article/10.1186/s40623-017-0722-3/fulltext.html
• 参照: Planetary-scale streak structure reproduced in a Venus atmospheric simulation; https://cir.nii.ac.jp/crid/1050012570393345792; Stationary Features at the Cloud Top of Venus Observed by Ultraviolet Imager Onboard Akatsuki; https://cir.nii.ac.jp/crid/1050856995322406656; Quasi‐Periodic Variation of the Lower Equatorial Cloud Induced by Atmospheric Waves on Venus; https://cir.nii.ac.jp/crid/1360013168842634624; Periodic Variation of Mesoscale Ultraviolet Contrast at the Cloud Top of Venus; https://cir.nii.ac.jp/crid/1360021389823062528; X-band scintillations in Venus radio occultations observed by Akatsuki; https://cir.nii.ac.jp/crid/1360025430213154560; Probing solar wind velocity from simultaneous superior solar conjunction radio science experiments of BepiColombo and Akatsuki missions; https://cir.nii.ac.jp/crid/1360025430652075648; Short vertical wavelength gravity waves in the Martian polar lower atmosphere observed by reanalysis of Mars Global Surveyor radio occultation data; https://cir.nii.ac.jp/crid/1360025430660345984; Lunar meter-wave telescope (TSUKUYOMI) as one of Japanese lunar plans; https://cir.nii.ac.jp/crid/1360025431125328000; Fine Vertical Structures at the Cloud Heights of Venus Revealed by Radio Holographic Analysis of Venus Express and Akatsuki Radio Occultation Data; https://cir.nii.ac.jp/crid/1360285708269382656; Horizontal structures of bow-shaped mountain wave trains seen in thermal infrared images of venusian clouds taken by Akatsuki LIR; https://cir.nii.ac.jp/crid/1360291932833393792; Gravity Wave Packets in the Venusian Atmosphere Observed by Radio Occultation Experiments: Comparison With Saturation Theory; https://cir.nii.ac.jp/crid/1360292617917737472; A Recharge Oscillator Model for Interannual Variability in Venus’ Clouds; https://cir.nii.ac.jp/crid/1360294643709230592; Dynamical Effect on Static Stability of the Venus Atmosphere Simulated Using a General Circulation Model: A Comparison With Radio Occultation Measurements; https://cir.nii.ac.jp/crid/1360298337072107520; Characteristic Features of <i>V</i>₀ Layer in the Venus Ionosphere as Observed by the Akatsuki Orbiter: Evidence for Its Presence During the Local Noon and Post‐Sunset Conditions; https://cir.nii.ac.jp/crid/1360298337072151040; Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind; https://cir.nii.ac.jp/crid/1360298757427814912; One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud Structure; https://cir.nii.ac.jp/crid/1360302864806108160; Density fluctuation in the solar corona and solar wind: A comparative analysis of radio-occultation observations and magnetohydrodynamic simulation; https://cir.nii.ac.jp/crid/1360306906087775488; Local Time Dependence of the Thermal Structure in the Venusian Equatorial Upper Atmosphere: Comparison of Akatsuki Radio Occultation Measurements and GCM Results; https://cir.nii.ac.jp/crid/1360567183246094848; Venusian Ionosphere During Deep Solar Minima: Some New Insights Using Akatsuki Radio Science Experiment; https://cir.nii.ac.jp/crid/1360579813137068160; Evaluation of new radio occultation observations among small satellites at Venus by data assimilation; https://cir.nii.ac.jp/crid/1360584340698593408; The nightside cloud-top circulation of the atmosphere of Venus; https://cir.nii.ac.jp/crid/1360853122781614336; Correlation of Venusian Mesoscale Cloud Morphology Between Images Acquired at Various Wavelengths; https://cir.nii.ac.jp/crid/1360861286472294016; Gravity Wave Modulations at the Lower Altitudes of Venus Ionosphere; https://cir.nii.ac.jp/crid/1360861289680250240; Thermal structure of the Venusian atmosphere from the sub-cloud region to the mesosphere as observed by radio occultation; https://cir.nii.ac.jp/crid/1361975843215420800; 惑星大気の衛星間電波掩蔽観測のための最適軌道に関する研究; https://cir.nii.ac.jp/crid/1390852581594739456; Venus Climate Orbiter Akatsuki RS Doppler Profiles PDS3 dataset; https://cir.nii.ac.jp/crid/1460002330940077696; Venus Climate Orbiter Akatsuki RS Bending Angle and Temperature/Pressure Profiles PDS3 dataset; https://cir.nii.ac.jp/crid/1460565280893499392; Evaluation of a method to retrieve temperature and wind velocity profiles of the Venusian nightside mesosphere from mid-infrared CO2 absorption line observed by heterodyne spectroscopy; https://cir.nii.ac.jp/crid/2050588892096576000; Ultraviolet imager on Venus orbiter Akatsuki and its initial results; https://cir.nii.ac.jp/crid/2051151842031753600; Special issue “Akatsuki at Venus : the first year of scientific operation”; https://cir.nii.ac.jp/crid/2051151842042436864; Influence of the cloud-level neutral layer on the vertical propagation of topographically generated gravity waves on Venus; https://cir.nii.ac.jp/crid/2051151842047685376
• 参照: Radio occultation measurement of the electron density near the lunar surface using a subsatellite on the SELENE mission; https://cir.nii.ac.jp/crid/1360002216708994560; Small-scale temperature fluctuations seen by the VeRa Radio Science Experiment on Venus Express; https://cir.nii.ac.jp/crid/1360004232184267520; Measurements of thermal structure and thermal contrasts in the atmosphere of Venus and related dynamical observations: Results From the four Pioneer Venus Probes; https://cir.nii.ac.jp/crid/1360011142930076160; The structure of Venus’ middle atmosphere and ionosphere; https://cir.nii.ac.jp/crid/1360011142932839680; Densities and temperatures in the Venus mesosphere and lower thermosphere retrieved from SOIR on board Venus Express: Carbon dioxide measurements at the Venus terminator; https://cir.nii.ac.jp/crid/1360011142937017856; Zonal Winds in the Middle Atmosphere of Venus from Pioneer Venus Radio Occultation Data; https://cir.nii.ac.jp/crid/1360011142937338752; The atmosphere of mars analyzed by integral inversion of the Mariner IV occultation data; https://cir.nii.ac.jp/crid/1360011142937660416; A Numerical Microphysical Model of the Condensational Venus Cloud; https://cir.nii.ac.jp/crid/1360011142940069760; Venus cloud formation in the meridional circulation; https://cir.nii.ac.jp/crid/1360011142941006848; Internal structure of a coronal mass ejection revealed by Akatsuki radio occultation observations; https://cir.nii.ac.jp/crid/1360285704780731904; Vertical Wavenumber Spectra of Gravity Waves in the Venus Atmosphere Obtained from Venus Express Radio Occultation Data: Evidence for Saturation; https://cir.nii.ac.jp/crid/1360285711534872832; H2O-H2SO4 System in Venus' Clouds and OCS, CO, and H2SO4 Profiles in Venus' Troposphere; https://cir.nii.ac.jp/crid/1360292617906610048; Vertical structure of the atmosphere of Venus from Pioneer Venus Orbiter radio occultations; https://cir.nii.ac.jp/crid/1360292617908724992; Greenhouse models of Venus' High surface temperature, as constrained by Pioneer Venus measurements; https://cir.nii.ac.jp/crid/1360292617908726400; Microwave absorptivity by sulfuric acid in the Venus atmosphere: First results from the Venus Express Radio Science experiment VeRa; https://cir.nii.ac.jp/crid/1360292617909416960; Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude; https://cir.nii.ac.jp/crid/1360292617911079424; Quantification of middle and lower cloud variability and mesoscale dynamics from Venus Express/VIRTIS observations at 1.74μm; https://cir.nii.ac.jp/crid/1360292617913589248; Magellan Radio Occultation Measurements of Atmospheric Waves on Venus; https://cir.nii.ac.jp/crid/1360292617914340608; Observable effects of convection and gravity waves on the Venus condensational cloud; https://cir.nii.ac.jp/crid/1360292617915273088; The Refractive Indices and Dielectric Constants of Air and its Principal Constituents at 24,000 Mc/s; https://cir.nii.ac.jp/crid/1360292617916322560; Radio Occultation Studies of the Venus Atmosphere with the Magellan Spacecraft; https://cir.nii.ac.jp/crid/1360292617917540864; RADIAL DISTRIBUTION OF COMPRESSIVE WAVES IN THE SOLAR CORONA REVEALED BY<i>AKATSUKI</i>RADIO OCCULTATION OBSERVATIONS; https://cir.nii.ac.jp/crid/1360565167378840064; Radio occultation measurements of turbulence in the Venus atmosphere by Pioneer Venus; https://cir.nii.ac.jp/crid/1360574092884442752; Dynamical properties of the Venus mesosphere from the radio-occultation experiment VeRa onboard Venus Express; https://cir.nii.ac.jp/crid/1360574092886126592; Radio Scintillations in Venus's Atmosphere: Application of a Theory of Gravity Wave Generation; https://cir.nii.ac.jp/crid/1360574092886548224; Radio science investigations by VeRa onboard the Venus Express spacecraft; https://cir.nii.ac.jp/crid/1360574092888752384; The Microwave Absorption and Abundance of Sulfuric Acid Vapor in the Venus Atmosphere Based on New Laboratory Measurements; https://cir.nii.ac.jp/crid/1360574092889418496; Statistical and computational uncertainties in atmospheric profiles from radio occultation: Mariner 10 at Venus; https://cir.nii.ac.jp/crid/1360574092891079680; The radio occultation method for the study of planetary atmospheres; https://cir.nii.ac.jp/crid/1360574092891082368; The Neutral Atmosphere of Venus as Studied with the Mariner V Radio Occultation Experiments; https://cir.nii.ac.jp/crid/1360574092891419392; Radio propagation experiments in the outer solar system with Voyager; https://cir.nii.ac.jp/crid/1360574092892323712; Modeling the effects of shear on the evolution of the holes in the condensational clouds of Venus; https://cir.nii.ac.jp/crid/1360574092892781184; Microphysics of Venusian Clouds in Rising Tropical Air; https://cir.nii.ac.jp/crid/1360574092893220992; OUTFLOW STRUCTURE OF THE QUIET SUN CORONA PROBED BY SPACECRAFT RADIO SCINTILLATIONS IN STRONG SCATTERING; https://cir.nii.ac.jp/crid/1360846642355362688; Inverse insolation dependence of Venus’ cloud-level convection; https://cir.nii.ac.jp/crid/1360848657114438272; Studying the Lunar Ionosphere with SELENE Radio Science Experiment; https://cir.nii.ac.jp/crid/1360855567865332480; The thermal structure of the Venus atmosphere: Intercomparison of Venus Express and ground based observations of vertical temperature and density profiles; https://cir.nii.ac.jp/crid/1360855567866207616; Solar cycle effects on the structure of the electron density profiles in the dayside ionosphere of Venus; https://cir.nii.ac.jp/crid/1360855567870392576; Structure of the Venus neutral atmosphere as observed by the Radio Science experiment VeRa on Venus Express; https://cir.nii.ac.jp/crid/1360855567871152000; Flight Model Development of PLANET-C Telecommunication Subsystem; https://cir.nii.ac.jp/crid/1390001205320835584; Venus Climate Orbiter Akatsuki RS Doppler Profiles PDS3 dataset; https://cir.nii.ac.jp/crid/1460002330940077696; Venus Climate Orbiter Akatsuki RS Bending Angle and Temperature/Pressure Profiles PDS3 dataset; https://cir.nii.ac.jp/crid/1460565280893499392; Overview of Venus orbiter, Akatsuki; https://cir.nii.ac.jp/crid/1523388080069817344; Radio occultation experiment of the Venus atmosphere and ionosphere with the Venus orbiter Akatsuki; https://cir.nii.ac.jp/crid/2050588892138311424; AKATSUKI returns to Venus; https://cir.nii.ac.jp/crid/2051714792052822656
• 連携機関・データベース: 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
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• 書誌ID（NDLBibID）: 11002663; http://id.ndl.go.jp/bib/11002663
• NII論文ID: 120006486821