Predicted thermal superluminescence in low-pressure air
It is shown that due to the dissociation of the molecular oxygen it is possible to obtain inverted population in low pressure air by heating. As a result of the quenching of the corresponding levels of the atomic oxygen the thermal superluminescent radiation is generated. It has been found that the...
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description | It is shown that due to the dissociation of the molecular oxygen it is possible to obtain inverted population in low pressure air by heating. As a result of the quenching of the corresponding levels of the atomic oxygen the thermal superluminescent radiation is generated. It has been found that the threshold of the overpopulation is exceeded at the air temperature 2300-3000 K. Using this effect a possible mechanism for the generation of the flashes of the radiation in air observed on the airframe of the space shuttle during its descent and reentry in the atmosphere is suggested. |
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As a result of the quenching of the corresponding levels of the atomic oxygen the thermal superluminescent radiation is generated. It has been found that the threshold of the overpopulation is exceeded at the air temperature 2300-3000 K. Using this effect a possible mechanism for the generation of the flashes of the radiation in air observed on the airframe of the space shuttle during its descent and reentry in the atmosphere is suggested.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.0909.2327</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Air temperature ; Airframes ; Atmospheric entry ; Atomic oxygen ; Low pressure ; Physics - Atmospheric and Oceanic Physics ; Physics - Atomic Physics ; Reentry</subject><ispartof>arXiv.org, 2009-09</ispartof><rights>2009. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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Using this effect a possible mechanism for the generation of the flashes of the radiation in air observed on the airframe of the space shuttle during its descent and reentry in the atmosphere is suggested.</description><subject>Air temperature</subject><subject>Airframes</subject><subject>Atmospheric entry</subject><subject>Atomic oxygen</subject><subject>Low pressure</subject><subject>Physics - Atmospheric and Oceanic Physics</subject><subject>Physics - Atomic Physics</subject><subject>Reentry</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2009</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotjztrwzAURkWh0JBm71QMne1e3StL1lhCH4FAO2Q3inVNHfyqZPfx75s0nb7l8HGOEDcSMlXkOdy78N18ZmDBZkhoLsQCiWRaKMQrsYrxAACoDeY5LYR5C-ybamKfTO8cOtcmcR45tHPX9Bwr7itOmj5ph690DBzjHDhxTbgWl7VrI6_-dyl2T4-79Uu6fX3erB-2qculSis0oIxGr2ukwhlgqSTp2psKmPa41ySNRZ8TWevQGsDa64qUBFAeLS3F7fn2L6ocQ9O58FOe4spT3BG4OwNjGD5mjlN5GObQH5VKhALJgEZFv-O5UDA</recordid><startdate>20090912</startdate><enddate>20090912</enddate><creator>Aramyan, A R</creator><creator>Haroyan, K P</creator><creator>Galechyan, G A</creator><creator>Mangasaryan, N R</creator><creator>Nersisyan, H B</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>GOX</scope></search><sort><creationdate>20090912</creationdate><title>Predicted thermal superluminescence in low-pressure air</title><author>Aramyan, A R ; Haroyan, K P ; Galechyan, G A ; Mangasaryan, N R ; Nersisyan, H B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-a514-c2704762d6f238a70e14136fd7c0e3b2b631792d53399a29702fd6c341004d293</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2009</creationdate><topic>Air temperature</topic><topic>Airframes</topic><topic>Atmospheric entry</topic><topic>Atomic oxygen</topic><topic>Low pressure</topic><topic>Physics - Atmospheric and Oceanic Physics</topic><topic>Physics - Atomic Physics</topic><topic>Reentry</topic><toplevel>online_resources</toplevel><creatorcontrib>Aramyan, A R</creatorcontrib><creatorcontrib>Haroyan, K P</creatorcontrib><creatorcontrib>Galechyan, G A</creatorcontrib><creatorcontrib>Mangasaryan, N R</creatorcontrib><creatorcontrib>Nersisyan, H B</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection><collection>arXiv.org</collection><jtitle>arXiv.org</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Aramyan, A R</au><au>Haroyan, K P</au><au>Galechyan, G A</au><au>Mangasaryan, N R</au><au>Nersisyan, H B</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Predicted thermal superluminescence in low-pressure air</atitle><jtitle>arXiv.org</jtitle><date>2009-09-12</date><risdate>2009</risdate><eissn>2331-8422</eissn><abstract>It is shown that due to the dissociation of the molecular oxygen it is possible to obtain inverted population in low pressure air by heating. As a result of the quenching of the corresponding levels of the atomic oxygen the thermal superluminescent radiation is generated. It has been found that the threshold of the overpopulation is exceeded at the air temperature 2300-3000 K. Using this effect a possible mechanism for the generation of the flashes of the radiation in air observed on the airframe of the space shuttle during its descent and reentry in the atmosphere is suggested.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.0909.2327</doi><oa>free_for_read</oa></addata></record> |
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subjects | Air temperature Airframes Atmospheric entry Atomic oxygen Low pressure Physics - Atmospheric and Oceanic Physics Physics - Atomic Physics Reentry |
title | Predicted thermal superluminescence in low-pressure air |
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