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

• Material Type: 記事
• Title: 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
• Author/Editor: Kosuke Takami; Hiromu Nakagawa; Hideo Sagawa
• Publication, Distribution, etc.: 日本 : Springer Nature
• Publication Date: 2020-05-07
• Publication Date (W3CDTF): 2020-05-07
• Periodical title: EPS : Earth, Planets and Space
• No. or year of volume/issue: 72(60)
• Volume: 72(60)
• ISSN (Periodical Title): 1880-5981
• ISSN-L (Periodical Title): 1343-8832
• Text Language Code: eng
• DOI: 10.1186/s40623-020-01188-0; https://doi.org/10.1186/s40623-020-01188-0
• Persistent ID (NDL): info:ndljp/pid/11520514; https://dl.ndl.go.jp/pid/11520514
• Collection: 障害者向け資料
• Collection (Materials For Handicapped People:1): テキストデータ
• 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; https://dl.ndl.go.jp/collections/B00035
• Acquisition Basis: オンライン資料収集制度
• Date Accepted (W3CDTF): 2020-08-03T12:00:21+09:00
• Date Captured (W3CDTF): 2020-08-03
• 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): https://earth-planets-space.springeropen.com/articles
• Periodical Title (Persistent ID (NDL)): info:ndljp/pid/11467692; https://dl.ndl.go.jp/pid/11467692
• 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; https://dl.ndl.go.jp

• 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/s40623-020-01188-0; https://doi.org/10.1186/s40623-020-01188-0
• Related Material: 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; https://cir.nii.ac.jp/crid/1881428068257760384
• Related Material (URI): http://id.ndl.go.jp/digimeta/11520514; https://dl.ndl.go.jp/pid/11520514; https://link.springer.com/content/pdf/10.1186/s40623-020-01188-0.pdf; https://link.springer.com/article/10.1186/s40623-020-01188-0/fulltext.html
• Is Referenced By: Mid-infrared laser heterodyne spectrometer by hollow optical fiber and its newly designed coupler; https://cir.nii.ac.jp/crid/1360861704769506816
• References: Initial performance of the radio occultation experiment in the Venus orbiter mission Akatsuki; https://cir.nii.ac.jp/crid/1050856995323578240; Mean winds at the cloud top of Venus obtained from two-wavelength UV imaging by Akatsuki; https://cir.nii.ac.jp/crid/1050856995323890688; Venus’ upper atmospheric dynamical structure from ground-based observations shortly before and after Venus’ inferior conjunction 2009; https://cir.nii.ac.jp/crid/1360004232184278912; 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; Circulation of the Venus upper mesosphere/lower thermosphere: Doppler wind measurements from 2001–2009 inferior conjunction, sub-millimeter CO absorption line observations; https://cir.nii.ac.jp/crid/1360011142932705152; The structure of Venus’ middle atmosphere and ionosphere; https://cir.nii.ac.jp/crid/1360011142932839680; A mechanism for the Venus thermospheric superrotation; https://cir.nii.ac.jp/crid/1360011142934567296; Net exchange parameterization of thermal infrared radiative transfer in Venus' atmosphere; https://cir.nii.ac.jp/crid/1360011142937011200; Modelling the atmospheric CO2 10-μm non-thermal emission in Mars and Venus at high spectral resolution; https://cir.nii.ac.jp/crid/1360011144526159744; Comparison of general circulation model atmospheric wave simulations with wind observations of venusian mesosphere; https://cir.nii.ac.jp/crid/1360285707160995200; IR heterodyne spectrometer MILAHI for continuous monitoring observatory of Martian and Venusian atmospheres at Mt. Haleakalā, Hawaii; https://cir.nii.ac.jp/crid/1360285707442187392; The HITRAN2012 molecular spectroscopic database; https://cir.nii.ac.jp/crid/1360292617907640064; Models of the structure of the atmosphere of Venus from the surface to 100 kilometers altitude; https://cir.nii.ac.jp/crid/1360292617911079424; Direct wind measurements from November 2007 in Venus’ upper atmosphere using ground-based heterodyne spectroscopy of CO2 at 10μm wavelength; https://cir.nii.ac.jp/crid/1360292618979661696; Aeronomy of the Venus Upper Atmosphere; https://cir.nii.ac.jp/crid/1360292621606271616; Long‐term variation in the cloud‐tracked zonal velocities at the cloud top of Venus deduced from Venus Express VMC images; https://cir.nii.ac.jp/crid/1360567183242856960; 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; Stationary waves and slowly moving features in the night upper clouds of Venus; https://cir.nii.ac.jp/crid/1360567183424826368; Cloud level winds from the Venus Express Monitoring Camera imaging; https://cir.nii.ac.jp/crid/1360574092890301824; Monitoring Venus’ mesospheric winds in support of Venus Express: IRAM 30-m and APEX observations; https://cir.nii.ac.jp/crid/1360574092891144832; Circulation of Venusian Atmosphere at 90–110 km Based on Apparent Motions of the O₂ 1.27 μm Nightglow From VIRTIS‐M (Venus Express) Data; https://cir.nii.ac.jp/crid/1360574092893479296; Temperatures in Venus upper atmosphere from mid-infrared heterodyne spectroscopy of CO2 around wavelength; https://cir.nii.ac.jp/crid/1360574095583080576; Absolute wind velocities in the lower thermosphere of Venus using infrared heterodyne spectroscopy; https://cir.nii.ac.jp/crid/1360574095723241984; The Level 2 research product algorithms for the Superconducting Submillimeter-Wave Limb-Emission Sounder (SMILES); https://cir.nii.ac.jp/crid/1360846646044524160; Effects of gravity waves on the day‐night difference of the general circulation in the Venusian lower thermosphere; https://cir.nii.ac.jp/crid/1360848655105934976; Doppler winds mapped around the lower thermospheric terminator of Venus: 2012 solar transit observations from the James Clerk Maxwell Telescope; https://cir.nii.ac.jp/crid/1360855567861049344; A dynamic upper atmosphere of Venus as revealed by VIRTIS on Venus Express; https://cir.nii.ac.jp/crid/1360855567862163968; Winds in the Middle Cloud Deck From the Near‐IR Imaging by the Venus Monitoring Camera Onboard Venus Express; https://cir.nii.ac.jp/crid/1360855567869369984; Thermal structure of the upper atmosphere of Venus simulated by a ground-to-thermosphere GCM; https://cir.nii.ac.jp/crid/1360855567870301568; Venus upper atmosphere winds from ground-based heterodyne spectroscopy of CO2 at wavelength; https://cir.nii.ac.jp/crid/1361981469916751232; Thermal structure of Venus׳ nightside mesosphere as observed by infrared heterodyne spectroscopy at 10 μm; https://cir.nii.ac.jp/crid/1361981471103207808; A warm layer in Venus' cryosphere and high-altitude measurements of HF, HCl, H2O and HDO; https://cir.nii.ac.jp/crid/1361981471420335744; Upper atmosphere temperature structure at the Venusian terminators: A comparison of SOIR and VTGCM results; https://cir.nii.ac.jp/crid/1362262943354161024; Thermal structure and CO distribution for the Venus mesosphere/lower thermosphere: 2001–2009 inferior conjunction sub-millimeter CO absorption line observations; https://cir.nii.ac.jp/crid/1362262945695541248; Long term evolution of temperature in the venus upper atmosphere at the evening and morning terminators; https://cir.nii.ac.jp/crid/1362544420228374528; Structure of the Venus mesosphere and lower thermosphere from measurements during entry of the pioneer Venus probes; https://cir.nii.ac.jp/crid/1362825893284780288; Thermospheric/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 techniques; https://cir.nii.ac.jp/crid/1363107369630218752; Wind mapping in Venus’ upper mesosphere with the IRAM-Plateau de Bure interferometer; https://cir.nii.ac.jp/crid/1363388845444282752; Direct observations of Venus upper mesospheric temperatures from ground based spectroscopy of CO₂; https://cir.nii.ac.jp/crid/1363388845481883392; Titan's stratospheric zonal wind, temperature, and ethane abundance a year prior to Huygens insertion; https://cir.nii.ac.jp/crid/1363388845963490304
• References (URI): https://cir.nii.ac.jp/crid/1370849946839576451
• Data Provider (Database): 国立情報学研究所 : CiNii Research; https://cir.nii.ac.jp/
• Original Data Provider (Database): 雑誌記事索引データベース; https://ndlsearch.ndl.go.jp; Crossref; https://www.crossref.org; 科学研究費助成事業データベース; https://kaken.nii.ac.jp/ja