<i>Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.</i>
One of the Orange Aid Preprint Series in Nuclear Astrophysics, September 1968.; Supported in part by the National Science Foundation [GP-7976], the Office of Naval Research [Nonr-220(47)]. ; ABSTRACT: The motion in a convectively unstable region is expanded into an ensemble of convective cells. Eac...
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University of Alabama in Huntsville Archives
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| Online Access: | http://libarchstor2.uah.edu/digitalcollections/items/show/10207 |
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Electronic |
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Saturn V Collection |
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University of Alabama in Huntsville Archives |
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University of Alabama in Huntsville Archives |
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Documents |
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Documents <i>Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.</i> Ulrich, Roger K. |
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Documents Saturn project Transport theory Convection Stellar atmospheres |
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One of the Orange Aid Preprint Series in Nuclear Astrophysics, September 1968.; Supported in part by the National Science Foundation [GP-7976], the Office of Naval Research [Nonr-220(47)]. ; ABSTRACT: The motion in a convectively unstable region is expanded into an ensemble of convective cells. Each of these cells interacts with the surrounding medium according to the semiempirical model proposed by Turner (1963 ). Possible detailed models of the flow patterns within each cell are presented. The radius and velocity of these cells are given as functions of distance moved. The convective flux and rms velocity are given as averages over the ensemble of cells. As in the standard mixing length theory the principle uncertainty remains the average initial radius of the cells. |
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<i>Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.</i>Ulrich, Roger K.Saturn projectTransport theoryConvectionStellar atmospheresOne of the Orange Aid Preprint Series in Nuclear Astrophysics, September 1968.; Supported in part by the National Science Foundation [GP-7976], the Office of Naval Research [Nonr-220(47)]. ; ABSTRACT: The motion in a convectively unstable region is expanded into an ensemble of convective cells. Each of these cells interacts with the surrounding medium according to the semiempirical model proposed by Turner (1963 ). Possible detailed models of the flow patterns within each cell are presented. The radius and velocity of these cells are given as functions of distance moved. The convective flux and rms velocity are given as averages over the ensemble of cells. As in the standard mixing length theory the principle uncertainty remains the average initial radius of the cells.1968-09-01TextEssaysConvenertranstel.pdfspc_stnv_000220http://libarchstor2.uah.edu/digitalcollections/items/show/10207http://libarchstor2.uah.edu/digitalcollections/files/original/20/10207/Convenertranstel_011509130952.pdfSaturn V CollectionBox 28, Folder 10University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabamaenspc_stnv_000200_000224This material may be protected under U. S. Copyright Law (Title 17, U.S. Code) which governs the making of photocopies or reproductions of copyrighted materials. You may use the digitized material for private study, scholarship, or research. Though the University of Alabama in Huntsville Archives and Special Collections has physical ownership of the material in its collections, in some cases we may not own the copyright to the material. It is the patron's obligation to determine and satisfy copyright restrictions when publishing or otherwise distributing materials found in our collections. |
| title |
<i>Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.</i> |
| titleStr |
<i>Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.</i> |
| author |
Ulrich, Roger K. |
| author_facet |
Ulrich, Roger K. |
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UAHsaturnv10207 |
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http://libarchstor2.uah.edu/digitalcollections/items/show/10207 |
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1790443372603768832 |