Pb isotopic signatures of the atmosphere of the São Paulo city, Brazil
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ADVERTISEMENT RETURN TO ISSUEPREVReportNEXTNature: Earth's Atmosphere and BeyondSabine Heinhorst and Gordon Cannon View Author Information Department of Chemistry and Biochemistry, University of Southern Mississippi, Hattiesburg, MS 39406-5043Cite this: J. Chem. Educ. 2003, 80, 10, 1115Publication Date (Web):October 1, 2003Publication History Received3 August 2009Published online1 October 2003Published inissue 1 October 2003https://pubs.acs.org/doi/10.1021/ed080p1115https://doi.org/10.1021/ed080p1115meeting-reportACS PublicationsRequest reuse permissionsArticle Views155Altmetric-Citations-LEARN ABOUT THESE METRICSArticle Views are the COUNTER-compliant sum of full text article downloads since November 2008 (both PDF and HTML) across all institutions and individuals. These metrics are regularly updated to reflect usage leading up to the last few days.Citations are the number of other articles citing this article, calculated by Crossref and updated daily. Find more information about Crossref citation counts.The Altmetric Attention Score is a quantitative measure of the attention that a research article has received online. Clicking on the donut icon will load a page at altmetric.com with additional details about the score and the social media presence for the given article. Find more information on the Altmetric Attention Score and how the score is calculated. Share Add toView InAdd Full Text with ReferenceAdd Description ExportRISCitationCitation and abstractCitation and referencesMore Options Share onFacebookTwitterWechatLinked InRedditEmail Other access optionsGet e-Alertsclose SUBJECTS:Chemical composition Get e-Alerts
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Despite its nearness, we know very little about the lunar atmosphere. Recent ground‐based observations, however, have increased our understanding of the atmosphere and our fascination with it. In the lunar atmosphere we can study important physical phenomena that also exist elsewhere in the solar system where they are not so easily examined. These phenomena also cannot be duplicated in terrestrial laboratories.
Solar atmosphere
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Research indicates that Earth’s moon once had an atmosphere comparable to the atmosphere of Mars today. The ancient lunar atmosphere could have weathered rocks, produced windstorms, and may be the source of the water found on the planetary body today.
Atmosphere of Mars
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Atmosphere of Venus
Atmosphere of Mars
Early Earth
Atmosphere of Earth
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In this work the general conditions for some bodies of a solar System (Mars atmosphere, high Earth's atmosphere, the near-surface atmosphere of comets) at which one is possible formation of ordered structures in dusty plasma of lightning's. Existence of discharges in a dust-atmosphere of comets and at dust storms on Mars while only conjecture, but, despite of it the author has found possible to discuss conditions of formation of ordered structures from charged microparticles on these bodies of a solar System. The estimations of dusty plasma parameters originating at such discharges are made. On the basis of these estimations is drawn a conclusion that the dusty plasma in conditions of a Mars atmosphere, gas-dusty atmosphere of comets and in high layers of a Earth's atmosphere, will have properties, close to properties of laboratory dust plasma, in which one the ordered structures from charged microparticles are supervised.© (2002) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Atmosphere of Mars
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Most of the masses accreting onto the earth and terrestrial planets impacted at sufficiently high velocities to release their volatiles into the atmosphere by impact-heating. However, based on models of planetary growth by accumulation from solid bodies, the time-scale for accretion was sufficiently long that the average surface temperatures could not have risen above 320 K. Using measured reaction rates, the released volatiles should have been re-incorporated into the planet by hydrating the surface minerals and were subsequently buried during accretion. Rapid hydration of impact products precludes the formation of a thick atmosphere as the planet accreted. Thus, only the subsequent differentiation and evolution of the terrestrial planets determined the size and composition of each planet's atmosphere.
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Бұл зерттеужұмысындaКaно моделітурaлы жәнеоғaн қaтыстытолықмәліметберілгенжәнеуниверситетстуденттерінебaғыттaлғaн қолдaнбaлы (кейстік)зерттеужүргізілген.АхметЯссaуи университетініңстуденттеріүшін Кaно моделіқолдaнылғaн, олaрдың жоғaры білімберусaпaсынa қоятынмaңыздытaлaптaры, яғнисaпaлық қaжеттіліктері,олaрдың мaңыздылығытурaлы жәнесaпaлық қaжеттіліктерінеқaтыстыөз университетінқaлaй бaғaлaйтындығытурaлы сұрaқтaр қойылғaн. Осы зерттеудіңмaқсaты АхметЯсaуи университетіндетуризмменеджментіжәнеқaржы бaкaлaвриaт бaғдaрлaмaлaрыныңсaпaсынa қaтыстыстуденттердіңқaжеттіліктерінaнықтaу, студенттердіңқaнaғaттaну, қaнaғaттaнбaу дәрежелерінбелгілеу,білімберусaпaсын aнықтaу мен жетілдіружолдaрын тaлдaу болыптaбылaды. Осы мaқсaтқaжетуүшін, ең aлдыменКaно сaуaлнaмaсы түзіліп,116 студенткеқолдaнылдыжәнебілімберугежәнеоның сaпaсынa қaтыстыстуденттердіңтaлaптaры мен қaжеттіліктерітоптықжұмыстaрaрқылыaнықтaлды. Екіншіден,бұл aнықтaлғaн тaлaптaр мен қaжеттіліктерКaно бaғaлaу кестесіменжіктелді.Осылaйшa, сaпa тaлaптaры төрт сaнaтқa бөлінді:болуытиіс, бір өлшемді,тaртымдыжәнебейтaрaп.Соңындa,қaнaғaттaну мен қaнaғaттaнбaудың мәндеріесептелдіжәнестуденттердіңқaнaғaттaну мен қaнaғaттaнбaу деңгейлерінжоғaрылaту мен төмендетудеосытaлaптaр мен қaжеттіліктердіңрөліaйқын aнықтaлды.Түйінсөздер:сaпa, сaпaлық қaжеттіліктер,білімберусaпaсы, Кaно моделі.
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The thermal structure of the upper atmosphere of Mars has been theoretically investigated. The exospheric temperature, for a pure CO2 model atmosphere, lies between 400° and 700°K. The origin of the Martian atmosphere is discussed in the light of these results.
Atmosphere of Mars
Exosphere
Atmospheric escape
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