Radiative heat transfer and hydrostatic stability in nocturnal fog
We have performed a one-dimensional and transient radiative heat transfer analysis in order to investigate interaction between atmospheric radiation and convective instability within a nocturnal fog. The radiation element method using the Ray Emission Model (REM^sup 2^), which is a generalized numer...
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| Veröffentlicht in: | Boundary-layer meteorology 2004-11, Vol.113 (2), p.273-286 |
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| creator | NISHIKAWA, Toru MARUYAMA, Shigenao SAKAI, Seigo |
| description | We have performed a one-dimensional and transient radiative heat transfer analysis in order to investigate interaction between atmospheric radiation and convective instability within a nocturnal fog. The radiation element method using the Ray Emission Model (REM^sup 2^), which is a generalized numerical method, in conjunction with a line-by-line (LBL) method, is employed to attain high spectral resolution calculations for anisotropically scattering fog. The results show that the convective instability has a strong dependence on radiative properties of the fog. For the condition of a 20-μm droplet diameter and liquid water content of 0.1 × 10^sup -3^ kg m^sup -3^;, the temperature profile within the fog becomes "S" shaped, and a convective instability layer forms in the middle or lower level of the fog. However, for the same water content and a 40-μm diameter droplet, no strong convective instability layer forms, whereas for a 10-μm diameter droplet a strong convective instability is observed.[PUBLICATION ABSTRACT] |
| doi_str_mv | 10.1023/B:BOUN.0000039376.13527.5e |
| format | Article |
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The radiation element method using the Ray Emission Model (REM^sup 2^), which is a generalized numerical method, in conjunction with a line-by-line (LBL) method, is employed to attain high spectral resolution calculations for anisotropically scattering fog. The results show that the convective instability has a strong dependence on radiative properties of the fog. For the condition of a 20-μm droplet diameter and liquid water content of 0.1 × 10^sup -3^ kg m^sup -3^;, the temperature profile within the fog becomes "S" shaped, and a convective instability layer forms in the middle or lower level of the fog. However, for the same water content and a 40-μm diameter droplet, no strong convective instability layer forms, whereas for a 10-μm diameter droplet a strong convective instability is observed.[PUBLICATION ABSTRACT]</description><identifier>ISSN: 0006-8314</identifier><identifier>EISSN: 1573-1472</identifier><identifier>DOI: 10.1023/B:BOUN.0000039376.13527.5e</identifier><identifier>CODEN: BLMEBR</identifier><language>eng</language><publisher>Dordrecht: Springer</publisher><subject>Atmosphere ; Earth, ocean, space ; Exact sciences and technology ; External geophysics ; Fog ; Heat transfer ; Meteorology ; Water content ; Water in the atmosphere (humidity, clouds, evaporation, precipitation)</subject><ispartof>Boundary-layer meteorology, 2004-11, Vol.113 (2), p.273-286</ispartof><rights>2004 INIST-CNRS</rights><rights>Kluwer Academic Publishers 2004</rights><lds50>peer_reviewed</lds50><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c380t-45004da38e33f41084299bfbc22c3ca5a5eee0cd11884efd61329bec41514c7d3</citedby><cites>FETCH-LOGICAL-c380t-45004da38e33f41084299bfbc22c3ca5a5eee0cd11884efd61329bec41514c7d3</cites></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>314,776,780,27901,27902</link.rule.ids><backlink>$$Uhttp://pascal-francis.inist.fr/vibad/index.php?action=getRecordDetail&idt=16179116$$DView record in Pascal Francis$$Hfree_for_read</backlink></links><search><creatorcontrib>NISHIKAWA, Toru</creatorcontrib><creatorcontrib>MARUYAMA, Shigenao</creatorcontrib><creatorcontrib>SAKAI, Seigo</creatorcontrib><title>Radiative heat transfer and hydrostatic stability in nocturnal fog</title><title>Boundary-layer meteorology</title><description>We have performed a one-dimensional and transient radiative heat transfer analysis in order to investigate interaction between atmospheric radiation and convective instability within a nocturnal fog. 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However, for the same water content and a 40-μm diameter droplet, no strong convective instability layer forms, whereas for a 10-μm diameter droplet a strong convective instability is observed.[PUBLICATION ABSTRACT]</description><subject>Atmosphere</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>External geophysics</subject><subject>Fog</subject><subject>Heat transfer</subject><subject>Meteorology</subject><subject>Water content</subject><subject>Water in the atmosphere (humidity, clouds, evaporation, precipitation)</subject><issn>0006-8314</issn><issn>1573-1472</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2004</creationdate><recordtype>article</recordtype><sourceid>BENPR</sourceid><recordid>eNqFkd9LwzAQx4MoOKf_QxnoW2uulzTp3uzwFwwH4p5Dmqauo2tn0wn77003YeCL93Ic97nvcfclZAI0AhrjfTbNFsu3iA6BKYokAuSxiLg9IyPgAkNgIj4nI99PQonALsmVc2tfCuB0RLJ3XVS6r75tsLK6D_pON660XaCbIljti651vW-bwKe8qqt-H1RN0LSm33WNroOy_bwmF6Wunb35zWOyfHr8mL2E88Xz6-xhHhqUtA8Zp5QVGqVFLBlQyeI0zcvcxLFBo7nm1lpqCgApmS2LBDBOc2sYcGBGFDgmd0fdbdd-7azr1aZyxta1bmy7cyqWKFki0n9BEAnlgAM4-QOu28NZTgn0apQL6aHpETL-F66zpdp21UZ3ewVUDSaoTA0mqJMJ6mCC4tYP3_5u0M7ouvTfNZU7KSQgUoAEfwCOPYfF</recordid><startdate>20041101</startdate><enddate>20041101</enddate><creator>NISHIKAWA, Toru</creator><creator>MARUYAMA, Shigenao</creator><creator>SAKAI, Seigo</creator><general>Springer</general><general>Springer Nature B.V</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>3V.</scope><scope>7TG</scope><scope>7TN</scope><scope>7UA</scope><scope>7XB</scope><scope>88F</scope><scope>88I</scope><scope>8FD</scope><scope>8FE</scope><scope>8FG</scope><scope>8FK</scope><scope>ABUWG</scope><scope>AEUYN</scope><scope>AFKRA</scope><scope>ARAPS</scope><scope>ATCPS</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>BHPHI</scope><scope>BKSAR</scope><scope>C1K</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>F1W</scope><scope>GNUQQ</scope><scope>H8D</scope><scope>H96</scope><scope>HCIFZ</scope><scope>KL.</scope><scope>L.G</scope><scope>L7M</scope><scope>M1Q</scope><scope>M2P</scope><scope>P5Z</scope><scope>P62</scope><scope>PATMY</scope><scope>PCBAR</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PYCSY</scope><scope>Q9U</scope><scope>7U5</scope></search><sort><creationdate>20041101</creationdate><title>Radiative heat transfer and hydrostatic stability in nocturnal fog</title><author>NISHIKAWA, Toru ; 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The radiation element method using the Ray Emission Model (REM^sup 2^), which is a generalized numerical method, in conjunction with a line-by-line (LBL) method, is employed to attain high spectral resolution calculations for anisotropically scattering fog. The results show that the convective instability has a strong dependence on radiative properties of the fog. For the condition of a 20-μm droplet diameter and liquid water content of 0.1 × 10^sup -3^ kg m^sup -3^;, the temperature profile within the fog becomes "S" shaped, and a convective instability layer forms in the middle or lower level of the fog. However, for the same water content and a 40-μm diameter droplet, no strong convective instability layer forms, whereas for a 10-μm diameter droplet a strong convective instability is observed.[PUBLICATION ABSTRACT]</abstract><cop>Dordrecht</cop><pub>Springer</pub><doi>10.1023/B:BOUN.0000039376.13527.5e</doi><tpages>14</tpages></addata></record> |
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| subjects | Atmosphere Earth, ocean, space Exact sciences and technology External geophysics Fog Heat transfer Meteorology Water content Water in the atmosphere (humidity, clouds, evaporation, precipitation) |
| title | Radiative heat transfer and hydrostatic stability in nocturnal fog |
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