Water vapor in the venus middle atmosphere
It is proposed that recent observations of water vapor abundances near 95 km altitude support the hypothesis that the aerosol particles in the upper haze layer of the Venus atmosphere are primarily concentrated sulfuric acid. Encrenaz et al. (1995) assumed the aerosol particles near 95 km altitude w...
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| Veröffentlicht in: | Advances in space research 1999, Vol.23 (9), p.1573-1576 |
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| container_title | Advances in space research |
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| creator | Mills, F.P. |
| description | It is proposed that recent observations of water vapor abundances near 95 km altitude support the hypothesis that the aerosol particles in the upper haze layer of the Venus atmosphere are primarily concentrated sulfuric acid. Encrenaz
et al. (1995) assumed the aerosol particles near 95 km altitude were water ice and inferred the temperature at that altitude was 140 ± 10 K. Their observations, however, may also be consistent with saturated water vapor over 70 – 75 wt% sulfuric acid for temperatures near the nominal 160 – 170 K. These two interpretations lead to significantly different predictions regarding the escape rate for hydrogen. |
| doi_str_mv | 10.1016/S0273-1177(99)00172-6 |
| format | Article |
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et al. (1995) assumed the aerosol particles near 95 km altitude were water ice and inferred the temperature at that altitude was 140 ± 10 K. Their observations, however, may also be consistent with saturated water vapor over 70 – 75 wt% sulfuric acid for temperatures near the nominal 160 – 170 K. These two interpretations lead to significantly different predictions regarding the escape rate for hydrogen.</description><identifier>ISSN: 0273-1177</identifier><identifier>EISSN: 1879-1948</identifier><identifier>DOI: 10.1016/S0273-1177(99)00172-6</identifier><language>eng</language><publisher>Elsevier Ltd</publisher><ispartof>Advances in space research, 1999, Vol.23 (9), p.1573-1576</ispartof><rights>1999</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c369t-9d7670c33793413101093984bd1183907752b3012f84d5d52d3f25fecb5a46b33</citedby><cites>FETCH-LOGICAL-c369t-9d7670c33793413101093984bd1183907752b3012f84d5d52d3f25fecb5a46b33</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktohtml>$$Uhttps://www.sciencedirect.com/science/article/pii/S0273117799001726$$EHTML$$P50$$Gelsevier$$H</linktohtml><link.rule.ids>314,776,780,3537,4010,27900,27901,27902,65306</link.rule.ids></links><search><creatorcontrib>Mills, F.P.</creatorcontrib><title>Water vapor in the venus middle atmosphere</title><title>Advances in space research</title><description>It is proposed that recent observations of water vapor abundances near 95 km altitude support the hypothesis that the aerosol particles in the upper haze layer of the Venus atmosphere are primarily concentrated sulfuric acid. Encrenaz
et al. (1995) assumed the aerosol particles near 95 km altitude were water ice and inferred the temperature at that altitude was 140 ± 10 K. Their observations, however, may also be consistent with saturated water vapor over 70 – 75 wt% sulfuric acid for temperatures near the nominal 160 – 170 K. These two interpretations lead to significantly different predictions regarding the escape rate for hydrogen.</description><issn>0273-1177</issn><issn>1879-1948</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>1999</creationdate><recordtype>article</recordtype><recordid>eNqFkE1LxDAQhoMouK7-BKEnUaGaSZqmOYksfsGCBxWPIU2mbKRfJt0F_73trnjd01ye952Zh5BzoDdAIb99o0zyFEDKS6WuKAXJ0vyAzKCQKgWVFYdk9o8ck5MYv0aISUln5PrTDBiSjem7kPg2GVaYbLBdx6TxztWYmKHpYr_CgKfkqDJ1xLO_OScfjw_vi-d0-fr0srhfppbnakiVk7mklnOpeAZ8vJAqroqsdAAFV1RKwUo-7q-KzAknmOMVExXaUpgsLzmfk4tdbx-67zXGQTc-Wqxr02K3jppJBgKyfC8IBVUZiAkUO9CGLsaAle6Db0z40UD1pFBvFerJj1ZKbxXqKXe3y-H47sZj0NF6bC06H9AO2nV-T8MvVj11eQ</recordid><startdate>1999</startdate><enddate>1999</enddate><creator>Mills, F.P.</creator><general>Elsevier Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>1999</creationdate><title>Water vapor in the venus middle atmosphere</title><author>Mills, F.P.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c369t-9d7670c33793413101093984bd1183907752b3012f84d5d52d3f25fecb5a46b33</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>1999</creationdate><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Mills, F.P.</creatorcontrib><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Advances in space research</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Mills, F.P.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Water vapor in the venus middle atmosphere</atitle><jtitle>Advances in space research</jtitle><date>1999</date><risdate>1999</risdate><volume>23</volume><issue>9</issue><spage>1573</spage><epage>1576</epage><pages>1573-1576</pages><issn>0273-1177</issn><eissn>1879-1948</eissn><abstract>It is proposed that recent observations of water vapor abundances near 95 km altitude support the hypothesis that the aerosol particles in the upper haze layer of the Venus atmosphere are primarily concentrated sulfuric acid. Encrenaz
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| issn | 0273-1177 1879-1948 |
| language | eng |
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| source | Elsevier ScienceDirect Journals |
| title | Water vapor in the venus middle atmosphere |
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