Thematische Bibliographien / Airglow Observations

Auswahl der wissenschaftlichen Literatur zum Thema „Airglow Observations“

Autor: Grafiati
Veröffentlicht am 4. Juni 2021
Zuletzt aktualisiert am 28. Januar 2023

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Inhaltsverzeichnis

  1. Zeitschriftenartikel
  2. Dissertationen
  3. Bücher
  4. Buchteile
  5. Konferenzberichte

Zeitschriftenartikel zum Thema "Airglow Observations":

1

Wüst, Sabine, Michael Bittner, Patrick J. Espy, W. John R. French und Frank J. Mulligan. „Hydroxyl airglow observations for investigating atmospheric dynamics: results and challenges“. Atmospheric Chemistry and Physics 23, Nr. 2 (27.01.2023): 1599–618. http://dx.doi.org/10.5194/acp-23-1599-2023.

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Abstract. Measurements of hydroxyl (OH*) airglow intensity are a straightforward and cost-efficient method which allows the derivation of information about the climate and dynamics of the upper mesosphere/lower thermosphere (UMLT) on different spatiotemporal scales during darkness. Today, instrument components can be bought “off-the-shelf” and developments in detector technology allows operation without cooling, or at least without liquid nitrogen cooling, which is difficult to automate. This makes instruments compact and suitable for automated operation. Here, we briefly summarize why an OH* airglow layer exists, how atmospheric dynamics influence it and how temperature can be derived from OH* airglow measurements. Then, we provide an overview of the scientific results regarding atmospheric dynamics (mainly gravity waves (GWs) but also planetary waves (PWs) and infrasound) achieved with OH* airglow measurements. We focus on long-term ground-based OH* airglow measurements or airglow measurements using a network of ground-based instruments. The paper includes further results from global or near-global satellite-based OH* airglow measurements, which are of special importance for characterizing the OH* airglow layer. Additionally, the results from the very few available airborne case studies using OH* airglow instruments are summarized. Scientific and technical challenges for the next few years are described.
2

Duann, Yi, Loren C. Chang, Chi-Yen Lin, Yueh-Chun Hsieh, Yun-Cheng Wen, Charles C. H. Lin und Jann-Yenq Liu. „A Methodology of Retrieving Volume Emission Rate from Limb-Viewed Airglow Emission Intensity by Combining the Techniques of Abel Inversion and Deep Learning“. Atmosphere 14, Nr. 1 (30.12.2022): 74. http://dx.doi.org/10.3390/atmos14010074.

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The conversion of airglow intensity to volume emission rate (VER) is a common method for studying the ionosphere, but the contribution of the intensity conversion process to the uncertainty in estimated electron or ion density is significant. The Abel inversion is a commonly used method for retrieving VERs from vertical profiles of airglow intensities accumulated along the rays horizontally at the tangent point, but it requires that the intensities converge to zero at their uppermost height, which is often not the case due to observational limitations. In this study, we present a method for optimizing the retrieval of VER from satellite-measured airglow intensities using the techniques of deep learning and Abel inversion. This method can be applied to fill in unobserved or discontinuous observations in airglow intensity profiles with the Chapman function, allowing them to be used with the Abel inversion to determine VERs. We validate the method using limb 135.6 nm airglow emission intensity data from the NASA Global-scale Observations of the Limb and Disk (GOLD) mission. Our training process involves using three hidden layers with varying numbers of neurons, and we compare the performance of the best-performing deep learning models to Abel-transformed results from real-time observations. The combination of Abel inversion and deep learning has the potential to optimize the process of converting intensity to VER and improve the capacity for analyzing ionospheric observations.
3

Huang, Tai-Yin. „Special Issue Editorial: Atmospheric Airglow—Recent Advances in Observations, Experimentations, and Modeling“. Atmosphere 12, Nr. 2 (03.02.2021): 202. http://dx.doi.org/10.3390/atmos12020202.

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4

Xu, J. Y., W. J. Liu, J. C. Bian, X. Liu, W. Yuan und C. Wang. „Method for retrieval of atmospheric water vapor using OH airglow for correction of astronomical observations“. Astronomy & Astrophysics 639 (Juli 2020): A29. http://dx.doi.org/10.1051/0004-6361/201834621.

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Context. Water vapor in the atmosphere undergoes quick spatial and temporal variations. This has a serious impact on ground-based astronomical observations from the visible band to the infrared band resulting from water vapor attenuation and emission. Aims. We seek to show how the sky spectrum of an astronomical observation can be used to determine the amount of precipitable water vapor (PWV) along the line of sight toward the science target. Methods. In this work, we discuss a method to retrieve the PWV from the OH(8-3) band airglow spectrum. We analyzed the influences of the pressure and temperature of the atmosphere and the different water vapor vertical distributions on the PWV retrieval method in detail. Meanwhile, the accuracy of the method was analyzed via Monte Carlo simulations. To further verify the method of PWV retrieval, we carried out cross comparisons between the PWV retrieved from OH airglow and PWV from the standard star spectra of UVES using equivalent widths of telluric absorption lines observed from 2000 to 2016 at Cerro Paranal in Chile. Results. The Monte Carlo tests and the comparison between the two different methods prove the availability the PWV retrieval method from OH airglow. These results show that using OH airglow spectra in astronomical observations, PWVs along the same line of sight as the astronomical observations can be retrieved in real time. Conclusions. We provide a quick and economical method for retrieving the water vapor along the same line of sight of astronomical observation in the real time. This is especially helpful to correcting the effect of water vapor on astronomical observations.
5

McDade, Ian C., und Edward J. Llewellyn. „Satellite airglow limb tomography: Methods for recovering structured emission rates in the mesospheric airglow layer“. Canadian Journal of Physics 71, Nr. 11-12 (01.11.1993): 552–63. http://dx.doi.org/10.1139/p93-084.

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In this paper, we investigate the possibility of using satellite airglow limb tomography to study spatial structures in the airglow emissions of the upper mesosphere and lower thermosphere. We describe inversion procedures for converting satellite airglow limb observations into two-dimensional distributions of volume emission rates. The performance of the inversion procedures is assessed using simulated limb observations and we demonstrate the potential of this tomographic technique for studying the horizontal and vertical characteristics of wave-driven disturbances in the 80–100 km region.
6

Sarkhel, Sumanta, Gunter Stober, Jorge L. Chau, Steven M. Smith, Christoph Jacobi, Subarna Mondal, Martin G. Mlynczak und James M. Russell III. „A case study of a ducted gravity wave event over northern Germany using simultaneous airglow imaging and wind-field observations“. Annales Geophysicae 40, Nr. 2 (22.03.2022): 179–90. http://dx.doi.org/10.5194/angeo-40-179-2022.

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Abstract. An intriguing and rare gravity wave event was recorded on the night of 25 April 2017 using a multiwavelength all-sky airglow imager over northern Germany. The airglow imaging observations at multiple altitudes in the mesosphere and lower thermosphere region reveal that a prominent upward-propagating wave structure appeared in O(1S) and O2 airglow images. However, the same wave structure was observed to be very faint in OH airglow images, despite OH being usually one of the brightest airglow emissions. In order to investigate this rare phenomenon, the altitude profile of the vertical wavenumber was derived based on colocated meteor radar wind-field and SABER temperature profiles close to the event location. The results indicate the presence of a thermal duct layer in the altitude range of 85–91 km in the southwest region of Kühlungsborn, Germany. Utilizing these instrumental data sets, we present evidence to show how a leaky duct layer partially inhibited the wave progression in the OH airglow emission layer. The coincidental appearance of this duct layer is responsible for the observed faint wave front in the OH airglow images compared O(1S) and O2 airglow images during the course of the night over northern Germany.
7

Maihara, Toshinori, Fumihide Iwamuro, Takuya Yamashita, Donald N. B. Hall, Lennox L. Cowie, Alan T. Tokunaga und Andrew Pickles. „Observations of the OH airglow emission“. Publications of the Astronomical Society of the Pacific 105 (September 1993): 940. http://dx.doi.org/10.1086/133259.

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8

Unterguggenberger, Stefanie, Stefan Noll, Wuhu Feng, John M. C. Plane, Wolfgang Kausch, Stefan Kimeswenger, Amy Jones und Sabine Moehler. „Measuring FeO variation using astronomical spectroscopic observations“. Atmospheric Chemistry and Physics 17, Nr. 6 (28.03.2017): 4177–87. http://dx.doi.org/10.5194/acp-17-4177-2017.

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Abstract. Airglow emission lines of OH, O2, O and Na are commonly used to probe the MLT (mesosphere–lower thermosphere) region of the atmosphere. Furthermore, molecules like electronically excited NO, NiO and FeO emit a (pseudo-) continuum. These continua are harder to investigate than atomic emission lines. So far, limb-sounding from space and a small number of ground-based low-to-medium resolution spectra have been used to measure FeO emission in the MLT. In this study the medium-to-high resolution echelle spectrograph X-shooter at the Very Large Telescope (VLT) in the Chilean Atacama Desert (24°37′ S, 70°24′ W; 2635 m) is used to study the FeO pseudo-continuum in the range from 0.5 to 0.72 µm based on 3662 spectra. Variations of the FeO spectrum itself, as well as the diurnal and seasonal behaviour of the FeO and Na emission intensities, are reported. These airglow emissions are linked by their common origin, meteoric ablation, and they share O3 as a common reactant. Major differences are found in the main emission peak of the FeO airglow spectrum between 0.58 and 0.61 µm, compared with a theoretical spectrum. The FeO and Na airglow intensities exhibit a similar nocturnal variation and a semi-annual seasonal variation with equinoctial maxima. This is satisfactorily reproduced by a whole atmosphere chemistry climate model, if the quantum yields for the reactions of Fe and Na with O3 are 13 ± 3 and 11 ± 2 % respectively. However, a comparison between the modelled O3 in the upper mesosphere and measurements of O3 made with the SABER satellite instrument suggests that these quantum yields may be a factor of ∼ 2 smaller.
9

Lee, Dae-Hee, Kwang-Il Seon, Jang-Hyun Park, Ho Jin, In-Soo Yuk, Uk-Won Nam, Won-Yong Han et al. „FIMS WAVELENGTH CALIBRATION VIA AIRGLOW LINE OBSERVATIONS“. Journal of Astronomy and Space Sciences 21, Nr. 4 (01.12.2004): 391–98. http://dx.doi.org/10.5140/jass.2004.21.4.391.

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10

López-Moreno, José J., Carmen Morales, José F. Gómez, Joaquín Trapero, Stuart Bowyer, Jerry Edelstein, Michael Lampton und Eric J. Korpela. „EURD observations of EUV nightime airglow lines“. Geophysical Research Letters 25, Nr. 15 (01.08.1998): 2937–40. http://dx.doi.org/10.1029/98gl52079.

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Die Auswahlen zum Thema "Airglow Observations" für konkrete Quellenarten können Sie auch interessieren:
Zeitschriftenartikel Dissertationen

Dissertationen zum Thema "Airglow Observations":

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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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 the intensities were 450 ± 50 R, 450 ± 20 R, 90 ± 20 R, 1620 ± 200 R, 970 ± 50 R, 680 ± 15 R, and 190 ± 20 R respectively. The OI 5577Å and 6300Å emissions were 320 ± 10 R and 160 ± 10 R respectively. These simultaneous emission intensities were compared with an atmospheric model which revealed that the O₂(A³Σ, A'³Δ, c¹Σ, b¹Σ) states and the OH(X²Π) state were heavily quenched. Analysis of the vibrational distributions of the O₂(A³Σ, A'³Δ, c¹Σ) states and the OH(X²Π) state, and dynamic intensity fluctuations of their related emission features provided independent confirmation of the conclusion that the O₂(A³ Σ, A'³Δ, c¹Σ) states and the OH(X²Π) state were heavily quenched.
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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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.
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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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.

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 northern Sweden. Each station is equipped with a sensitive high-resolution (1024 x 1024 pixels) unintensified monochromatic CCDimager. A six-position filter-wheel for narrow-band interference filters facilitates absolute spectroscopic measurements of, for example, auroral and airglow emissions. Overlapping fields-of-view resulting from the station baseline of about 50 km combined with the station field-of-view of 50° to 60°, enable triangulation as well as tomographic methods to be employed for obtaining altitude information of the observed phenomena.

ALIS was probably one of the first instruments to take advantage of unintensi- fied (i.e. no image-intensifier) scientific-grade CCDs as detectors for spectroscopic imaging studies with multiple stations of faint phenomena such as aurora, airglow, etc. This makes absolute calibration a task that is as important as it is dificult.

Although ALIS was primarily designed for auroral studies, the majority of the scientific results so far have, quite unexpectedly, been obtained from observations of HF pump-enhanced airglow (recently renamed Radio-Induced Aurora). ALIS made the first unambiguous observation of this phenomena at high-latitudes and the first tomography-like inversion of height profiles of the airglow regions. The scientific results so far include tomographic estimates of the auroral electron spectra, coordinated observations with satellite and radar, as well as studies of polar stratospheric clouds. An ALIS imager also participated in a joint project that produced the first ground-based daytime auroral images. Recently ALIS made spectroscopic observations of a Leonid meteor-trail and preliminary analysis indicates the possible detection of water in the Leonid.

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
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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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.
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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Bücher zum Thema "Airglow Observations":

1

A, Kiselev V. Modelʹ ėmissiĭ ionov N⁺₂ i O⁺ dnevnoĭ atmosfery. Moskva: Moskovskoe otd-nie Gidrometeoizdata, 1986.

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E, Sharp W., und United States. National Aeronautics and Space Administration., Hrsg. An assessment of twilight airglow inversion procedures using atmosphere Explorer observations. [Washington, DC: National Aeronautics and Space Administration, 1993.

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E, Sharp W., und United States. National Aeronautics and Space Administration., Hrsg. An assessment of twilight airglow inversion procedures using atmosphere Explorer observations. [Washington, DC: National Aeronautics and Space Administration, 1993.

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Yao, I. G. Observations of the Night Airglow: 1 July 1957--31 December 1959. Elsevier Science & Technology Books, 2013.

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1929-, Nikolaev A. G., Riǐves L. I͡A︡ und Astrofüüsika ja Atmosfäärifüüsika Institut (Eesti NSV Teaduste Akadeemia), Hrsg. Issledovanii͡a︡ atmosfery i zemnoĭ poverkhnosti iz kosmosa. Tartu: Akademii͡a︡ nauk Ėstonskoĭ SSR, 1988.

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Buchteile zum Thema "Airglow Observations":

1

HOFFMEISTER, C., und J. PATON. „VISUAL OBSERVATIONS OF THE AIRGLOW AND OTHER NON-AURORAL LUMINOSITIES OF THE NIGHT SKY“. In Nuclear Radiation, 110–14. Elsevier, 2013. http://dx.doi.org/10.1016/b978-1-4832-1337-8.50014-0.

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ROACH, F. E. „PHOTOMETRIC OBSERVATION OF THE AIRGLOW“. In Nuclear Radiation, 115–38. Elsevier, 2013. http://dx.doi.org/10.1016/b978-1-4832-1337-8.50015-2.

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Konferenzberichte zum Thema "Airglow Observations":

1

Bobik, Pavol, Ondrej Matija, Marián Putiš, Frantisek Koval, Michal Vrábel, Simon Mackovjak, Jan Genci, Kenji Shinozaki, Mario E. Bertaina und Francesco Fenu. „Airglow dynamics observations by Mini-EUSO“. In 35th International Cosmic Ray Conference. Trieste, Italy: Sissa Medialab, 2017. http://dx.doi.org/10.22323/1.301.0408.

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2

Carlesso, Pablo Fernando, Marcelo Barcellos da Rosa, Nelson Jorge Schuch, Delano Gobbi, Hisao Takahashi und Makita Kasuo. „Airglow observations in the region of South Atlantic magnetic anomaly“. In 10th International Congress of the Brazilian Geophysical Society & EXPOGEF 2007, Rio de Janeiro, Brazil, 19-23 November 2007. Society of Exploration Geophysicists and Brazilian Geophysical Society, 2007. http://dx.doi.org/10.1190/sbgf2007-403.

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Fernando Carlesso, Pablo, Marcelo Barcellos da Rosa, Nelson Jorge Schuch, Delano Gobbi, Hisao Takahashi und Makita Kasuo. „Airglow observations in the region of South Atlantic magnetic anomaly“. In 10th International Congress of the Brazilian Geophysical Society. European Association of Geoscientists & Engineers, 2007. http://dx.doi.org/10.3997/2214-4609-pdb.172.sbgf0426_07.

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N., Venkataramanaiah, Varadarajan S. und Ramkumar T.K. „Automatic Dynamical Airglow Observations By All-Sky Images From Gadanki,India“. In 2019 IEEE International Conference on Electrical, Computer and Communication Technologies (ICECCT). IEEE, 2019. http://dx.doi.org/10.1109/icecct.2019.8869471.

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Coakley, Monica M., und Fred L. Roesler. „Application of conventional CCD cameras with Fabry-Perot spectrometers for airglow observations“. In SPIE's 1994 International Symposium on Optics, Imaging, and Instrumentation, herausgegeben von Jinxue Wang und Paul B. Hays. SPIE, 1994. http://dx.doi.org/10.1117/12.187548.

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Dayton, David C., Jeffery Allen, Rudolph Nolasco, John D. Gonglewski, Michael Myers, Dennis Burns, Ishan Mons und Francisco Maia. „Passive SWIR airglow illuminated imaging compared with NIR-visible for low-light nighttime observations“. In SPIE Defense, Security, and Sensing. SPIE, 2011. http://dx.doi.org/10.1117/12.884233.

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Saunkin, Andrei, Roman Vasilyev und Olga Zorkaltseva. „Airglow intensity of atomic oxygen 557.7 nm according to satellite and ground-based observations over Eastern Siberia“. In 27th International Symposium on Atmospheric and Ocean Optics, Atmospheric Physics, herausgegeben von Oleg A. Romanovskii und Gennadii G. Matvienko. SPIE, 2021. http://dx.doi.org/10.1117/12.2603386.

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Medvedeva, Irina, und Anatoly Semenov. „Studying MLT temperature and composition during stratospheric warming events from spectrometric observations of OH (6-2) airglow emission at mid-latitudes“. In XXIV International Symposium, Atmospheric and Ocean Optics, Atmospheric Physics, herausgegeben von Oleg A. Romanovskii und Gennadii G. Matvienko. SPIE, 2018. http://dx.doi.org/10.1117/12.2504553.

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Buriti, R. A., H. Takahashi und D. Gobbi. „First Oi6300 And Oi5577 Airglow Observation Results From 7.5S“. In 6th International Congress of the Brazilian Geophysical Society. European Association of Geoscientists & Engineers, 1999. http://dx.doi.org/10.3997/2214-4609-pdb.215.sbgf188.

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Tu, Cui, Xiong Hu, Shangyong Guo, Zhaoai Yan und Yongqiang Cheng. „CSSAR airglow gravity wave imager and its preliminary observation“. In International Symposium on Photoelectronic Detection and Imaging 2009, herausgegeben von Kun Zhang, Xiang-jun Wang, Guang-jun Zhang und Ke-cong Ai. SPIE, 2009. http://dx.doi.org/10.1117/12.835580.

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