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
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DOI[10.1186/s40623-020-01188-0]のデータに遷移します
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- 資料種別
- 記事
- 著者・編者
- Kosuke TakamiHiromu NakagawaHideo Sagawa
- 出版年月日等
- 2020-05-07
- 出版年（W3CDTF）
- 2020-05-07
- タイトル（掲載誌）
- EPS : Earth, Planets and Space
- 巻号年月日等（掲載誌）
- 72(60)
- 掲載巻
- 72(60)
- 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/s40623-020-01188-0
- 国立国会図書館永続的識別子
- info:ndljp/pid/11520514
- 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）
- 2020-08-03T12:00:21+09:00
- 保存日（W3CDTF）
- 2020-08-03
- 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/11467692
- 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/s40623-020-01188-0
- 関連情報
- Additional file 1 of 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
- 関連情報（URI）
- 参照
- Mid-infrared laser heterodyne spectrometer by hollow optical fiber and its newly designed coupler
- 参照
- Initial 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 AkatsukiVenus’ upper atmospheric dynamical structure from ground-based observations shortly before and after Venus’ inferior conjunction 2009Measurements of thermal structure and thermal contrasts in the atmosphere of Venus and related dynamical observations: Results From the four Pioneer Venus ProbesCirculation of the Venus upper mesosphere/lower thermosphere: Doppler wind measurements from 2001–2009 inferior conjunction, sub-millimeter CO absorption line observationsThe structure of Venus’ middle atmosphere and ionosphereA mechanism for the Venus thermospheric superrotationNet exchange parameterization of thermal infrared radiative transfer in Venus' atmosphereModelling the atmospheric CO2 10-μm non-thermal emission in Mars and Venus at high spectral resolutionComparison of general circulation model atmospheric wave simulations with wind observations of venusian mesosphereIR heterodyne spectrometer MILAHI for continuous monitoring observatory of Martian and Venusian atmospheres at Mt. Haleakalā, HawaiiThe HITRAN2012 molecular spectroscopic databaseModels of the structure of the atmosphere of Venus from the surface to 100 kilometers altitudeDirect wind measurements from November 2007 in Venus’ upper atmosphere using ground-based heterodyne spectroscopy of CO2 at 10μm wavelengthAeronomy of the Venus Upper AtmosphereLong‐term variation in the cloud‐tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC imagesLocal 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 VenusCloud level winds from the Venus Express Monitoring Camera imagingMonitoring Venus’ mesospheric winds in support of Venus Express: IRAM 30-m and APEX observationsCirculation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O<sub>2</sub> 1.27 μm Nightglow From VIRTIS‐M (Venus Express) DataTemperatures in Venus upper atmosphere from mid-infrared heterodyne spectroscopy of CO2 around wavelengthAbsolute wind velocities in the lower thermosphere of Venus using infrared heterodyne spectroscopyThe Level 2 research product algorithms for the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES)Effects of gravity waves on the day‐night difference of the general circulation in the Venusian lower thermosphereDoppler winds mapped around the lower thermospheric terminator of Venus: 2012 solar transit observations from the James Clerk Maxwell TelescopeA dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus ExpressWinds in the Middle Cloud Deck From the Near‐IR Imaging by the Venus Monitoring Camera Onboard Venus ExpressThermal structure of the upper atmosphere of Venus simulated by a ground-to-thermosphere GCMVenus upper atmosphere winds from ground-based heterodyne spectroscopy of CO2 at wavelengthThermal structure of Venus׳ nightside mesosphere as observed by infrared heterodyne spectroscopy at 10 μmA warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDOUpper atmosphere temperature structure at the Venusian terminators: A comparison of SOIR and VTGCM resultsThermal structure and CO distribution for the Venus mesosphere/lower thermosphere: 2001–2009 inferior conjunction sub-millimeter CO absorption line observationsLong term evolution of temperature in the venus upper atmosphere at the evening and morning terminatorsStructure of the Venus mesosphere and lower thermosphere from measurements during entry of the pioneer Venus probesThermospheric/mesospheric temperatures on Venus: Results from ground-based high-resolution spectroscopy of CO2 in 1990/1991 and comparison to results from 2009 and between other techniquesWind mapping in Venus’ upper mesosphere with the IRAM-Plateau de Bure interferometerDirect observations of Venus upper mesospheric temperatures from ground based spectroscopy of CO<sub>2</sub>Titan's stratospheric zonal wind, temperature, and ethane abundance a year prior to Huygens insertion
- 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
- 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Crossref
- 書誌ID（NDLBibID）
- 11520514