Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.
Item
Dublin Core
Identifier
Convenertranstel.pdf
spc_stnv_000220
Title
Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.
Alternative Title
OAP - 143.
Description
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.
Creator
Date
1968-09-01
Temporal Coverage
Source
Saturn V Collection
Box 28, Folder 10
University of Alabama in Huntsville Archives, Special Collections, and Digital Initiatives, Huntsville, Alabama
Language
Rights
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Relation
spc_stnv_000200_000224
Is Referenced By
<a href="http://libarchstor.uah.edu:8081/repositories/2/archival_objects/17952">View this item at ArchivesSpace </a>
Collection
Citation
Ulrich, Roger K., “Convective Energy Transport in Stellar Atmospheres: A Convective Cell Model.,” UAH Archives, Special Collections, and Digital Initiatives, accessed December 24, 2024, http://libarchstor2.uah.edu/digitalcollections/items/show/11083.