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Tesi sul tema "Airglow Observations"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 28 gennaio 2023

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1

Greet, P. A. "Observations on the sodium airglow /." Title page, contents and abstract only, 1988. http://web4.library.adelaide.edu.au/theses/09PH/09phg8166.pdf.

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2

Johnston, Jeffrey Eric. "Spectroscopic observations of the night airglow from 3000 Å to 9200 Å." Diss., The University of Arizona, 1992. http://hdl.handle.net/10150/185790.

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Spectroscopic measurements of the night airglow were taken at mid latitude over a period of four months. The use of intensified CCD spectrographs allowed simultaneous data to be taken from 3000Å to 9200Å in 3300 contiguous spectral elements with a resolution (full width at half max.) of 6Å to 15Å. The average intensities for a 6.5 hour integration period on March 16, 1991 of the O₂ Herzberg I, Chamberlain, Herzberg II, and Atmospheric (0-1) emissions were 230 ± 20 R, 80 ± 10 R, 80 ± 40 R, and 350 ± 20 R respectively. For the OH Meinel (9-4), (8-3), (7-2), (7-3), (6-2), (5-1), (4-0) emissions t

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3

Song, Rui [Verfasser]. "Tomographic reconstruction of gravity wave parameters from satellite-borne airglow observations / Rui Song." Wuppertal : Universitätsbibliothek Wuppertal, 2018. http://d-nb.info/1156625394/34.

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4

Hozumi, Yuta. "Study on dynamics in the mesosphere, thermosphere and ionosphere with optical observations from the International Space Station." 京都大学 (Kyoto University), 2017. http://hdl.handle.net/2433/225411.

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5

Woithe, Jonathan Mark. "Optical studies of the mesospheric region." Title page, contents and abstract only, 2000. http://web4.library.adelaide.edu.au/theses/09PH/09phw847.pdf.

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Includes copies of articles co-authored by the author during the preparation of this thesis. Includes bibliographical references (leaves 233-245). A three-field photometer was employed at the University of Adelaide's Buckland Park field site to collect optical observations of the 557.7nm OI and 730nm OH airglow emissions on an almost continuous basis since May 1995 to May 2000, with observations made whenever the moon was not up.

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6

Brändström, Urban. "The Auroral Large Imaging System : design, operation and scientific results." Doctoral thesis, Umeå University, Space Science, 2003. http://urn.kb.se/resolve?urn=urn:nbn:se:umu:diva-36.

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<p>The Auroral Large Imaging System (ALIS) was proposed in 1989 by Åke Steen as a joint Scandinavian ground-based nework of automated auroral imaging stations. The primary scientic objective was in the field of auroral physics, but it was soon realised that ALIS could be used in other fields, for example, studies of Polar Stratospheric Clouds (PSC), meteors, as well as other atmospheric phenomena.</p><p>This report describes the design, operation and scientic results from a Swedish prototype of ALIS consisting of six unmanned remote-controlled stations located in a grid of about 50 km in north

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7

Akiya, Yusuke. "Visible and near-infrared airglow structures in the mesosphere and the lower thermosphere observed by space-borne instruments." 京都大学 (Kyoto University), 2015. http://hdl.handle.net/2433/199107.

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8

LE, TEXIER-COULOMB HELENE. "Etude des composes de l'hydrogene, ch4, h2o, h2 et hox dans la stratosphere et la mesosphere : photochimie et transport." Paris 7, 1987. http://www.theses.fr/1987PA077275.

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Le cycle des composes de l'hydrogene dans la stratosphere et la mesosphere est etudie a l'aide d'un modele numerique 2d. La premiere partie est consacree a l'etude du bilan de la vapeur d'eau, avec un traitement detaille de sa production par l'oxydation du methane et de l'hydrogene moleculaire. Dans la seconde partie, le mecanisme photochimique et la variabilite saisonniere de l'emission mesospherique de oh dans les bandes de meinel sont abordes d'un point de vue theorique

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9

Greet, P. A. (Penelope A. ). "Observations on the sodium airglow." 1988. http://web4.library.adelaide.edu.au/theses/09PH/09phg8166.pdf.

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10

Babcock, David D. "Mesospheric Imaging Michelson Interferometer instrument development and observations /." 2006. http://proquest.umi.com/pqdweb?index=1&did=1251892871&SrchMode=1&sid=3&Fmt=2&VInst=PROD&VType=PQD&RQT=309&VName=PQD&TS=1195659544&clientId=5220.

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Thesis (Ph.D.)--York University, 2006. Graduate Programme in Earth and Space Science.<br>Typescript. Includes bibliographical references (leaves 144-148). Also available on the Internet. MODE OF ACCESS via web browser by entering the following URL: http://proquest.umi.com/pqdweb?index=1&did=1251892871&SrchMode=1&sid=3&Fmt=2&VInst=PROD&VType=PQD&RQT=309&VName=PQD&TS=1195659544&clientId=5220

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11

Duann, Yi, and 段儀. "Photochemical model for atomic oxygen ion retrieval from ground-based observations of airglow." Thesis, 2018. http://ndltd.ncl.edu.tw/handle/r8awyq.

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碩士<br>國立中央大學<br>太空科學研究所<br>106<br>To study the chemistry and composition of the upper atmosphere, we can utilize airglow emissions from the photochemical reactions of the ions in this region. When the atomic oxygen ions distributed in the ionospheric F region experience an energy level transition, visible light with a wavelength of 630.0 nm is released. We used the photometer system built by our team at NCU to perform ground-based observations of airglow over the sky of Taiwan at Lulin Observatory (23.46°N, 120.87°E) during selected night times. Ground-based airglow spectrometer observations t

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12

Anderson, David Scott. "Estimation of intrinsic gravity wave parameters from multiple, ground-based observations of a single mesopheric airglow emission /." 2008. http://gateway.proquest.com/openurl?url_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:dissertation&res_dat=xri:pqdiss&rft_dat=xri:pqdiss:3337685.

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Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2008.<br>Source: Dissertation Abstracts International, Volume: 69-11, Section: B, page: 7015. Adviser: Gary R. Swenson. Includes bibliographical references (leaves 105-108) Available on microfilm from Pro Quest Information and Learning.

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13

Liu, Ker-Wei, and 劉格瑋. "Long Term Correlation Study of Observations Between FORMOSAT-2/ISUAL 6300A Airglow and FORMOSAT-3/GOX Electron Density." Thesis, 2009. http://ndltd.ncl.edu.tw/handle/25949043924084981205.

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碩士<br>國立成功大學<br>物理學系碩博士班<br>97<br>The atomic oxygen red line (6300A) is one of the strongest features in the visible nighttime airglow spectrum at low latitudes which comes from dissociative recombination of the molecular oxygens and electrons. In this study, ionospheric airglows in 6300A wavelength observed by the Imager of Sprites and Upper Atmospheric Lightning (ISUAL) on board the FORMOSAT-2 satellite are used to obtain their long term correlation with the global three-dimensional electron density structure obtained by the radio occultation experiment (GOX) of the FORMOSAT-3/COSMIC satelli

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14

McIntosh, Daniel L. "Comparisons of VHF meteor radar observations in the middle atmosphere with multiple independent remote sensing techniques." 2010. http://hdl.handle.net/2440/60068.

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This thesis describes the development, modification and refinement of a high-powered hybrid Stratospheric Tropospheric (ST)/meteor radar at the University of Adelaide’s Buckland Park (BP) field station. This thesis also describes the process of statistically comparing results obtained from multiple co-located independent measurement sources. Also included are statistical comparisons made between meteor radars at BP,Darwin, Northern Territory, and Davis Station, Antarctica, with other independent sources of measurement. Previous meteor radar systems have generally been low powered (∼8 kW peak)

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15

McIntosh, Daniel L. "Comparisons of VHF meteor radar observations in the middle atmosphere with multiple independent remote sensing techniques." Thesis, 2010. http://hdl.handle.net/2440/60068.

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Abstract (sommario):

This thesis describes the development, modification and refinement of a high-powered hybrid Stratospheric Tropospheric (ST)/meteor radar at the University of Adelaide’s Buckland Park (BP) field station. This thesis also describes the process of statistically comparing results obtained from multiple co-located independent measurement sources. Also included are statistical comparisons made between meteor radars at BP,Darwin, Northern Territory, and Davis Station, Antarctica, with other independent sources of measurement. Previous meteor radar systems have generally been low powered (∼8 kW peak)

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16

Liao, Cang-Hsien, and 廖昌賢. "Observation of Equatorial Plasma Depletions at Southern Taiwan by 6300Å OI Airglow." Thesis, 2000. http://ndltd.ncl.edu.tw/handle/00953787269318948067.

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碩士<br>國立中山大學<br>物理學系研究所<br>88<br>Abstract In this study, we use a fisheye lens (180o field of view) and Chare-Couple Device to take the all-sky 6300Å airglow images emitting from ionosphere. By analyzing these Images we can study the phenomenon of equatorial plasma depletions (plasma bubble). Plasma bubbles generate above the magnetic equator; and they drift up to higher altitude and spread to higher latitude area along magnetic lines. The all-sky imaging system was operated at Mt. A-Li (23.511oN, 120.823oE). Because this year is the most active time of sunspots in the solar cycle, we expect

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