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	<title>Электронный научно-практический журнал «Современные научные исследования и инновации» &#187; the internal sources of the heat</title>
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		<title>Моделирование теплообмена в зоне субдукции. Часть I</title>
		<link>https://web.snauka.ru/issues/2016/03/65807</link>
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		<pubDate>Wed, 02 Mar 2016 11:57:54 +0000</pubDate>
		<dc:creator>Соловьев Сергей Викторович</dc:creator>
				<category><![CDATA[01.00.00 ФИЗИКО-МАТЕМАТИЧЕСКИЕ НАУКИ]]></category>
		<category><![CDATA[convective heat transfer]]></category>
		<category><![CDATA[Earth's mantle]]></category>
		<category><![CDATA[modeling]]></category>
		<category><![CDATA[subduction]]></category>
		<category><![CDATA[the internal sources of the heat]]></category>
		<category><![CDATA[the lithosphere]]></category>
		<category><![CDATA[внутренние источники тепла]]></category>
		<category><![CDATA[конвективный теплообмен]]></category>
		<category><![CDATA[литосфера]]></category>
		<category><![CDATA[мантия Земли]]></category>
		<category><![CDATA[моделирование]]></category>
		<category><![CDATA[субдукция]]></category>

		<guid isPermaLink="false">https://web.snauka.ru/issues/2016/03/65807</guid>
		<description><![CDATA[1. Introduction  In article [1] presents an overview of the state of immersion and convective heat transfer problems lithospheric plate in the subduction zone. In spite of a great number of publications dealing with a study of the natural mantle convection, the questions concerning the character, structure and the primary reason for occurrence of the [...]]]></description>
			<content:encoded><![CDATA[<p><strong><span>1. Introduction </span></strong></p>
<p><span>In article [1] presents an overview of the state of immersion and convective heat transfer problems lithospheric plate in the subduction zone. In spite of a great number of publications dealing with a study of the natural mantle convection, the questions concerning the character, structure and the primary reason for occurrence of the convection remain still open. In fact, the influence of convection on the geometry of plates and, also, differences in the character of convection caused by using the Newtonian and non-Newtonian models of Earth’s mantle, has not been studied yet.</span><br />
<span>Undoubtedly, solution of these questions will entail great difficulties as at the stage of setting the problems so at the stage of their numerical solution. The above difficulties are caused by non-linearity of the problem, that is, the temperature and pressure dependence, practically, of all parameters of the mantle, lack of information on a lot of rheological parameters, restriction to the stability of the numerical solution due to prevalence of viscosity members over the inertial ones in the Navier-Stokes equations.</span><br />
<span>The main shortcoming of the above mathematical models is the fact that phases transitions at 670 km depth causing jumps in viscosity and density of the mantle substance which, in the opinion of some researchers, may lead to localization of the convection in the upper mantle, are not taken into account.</span></p>
<p><strong><span>2. Formulation of the Problem</span></strong></p>
<p><span>The paper considers a 2-D model of the continuous convection of the lithospheric plate close to oceanic trench with regard for the heat of the phase transition. The subduction zone is considered, where lithospheric plate collides with continental, and then on a trough, which axis is located under an angle to the land surface, is immersed in mantle. The depth of immersing of lithospheric plate in mantle is determined as a result of the task decision. Constructing the mathematical model, the following assumptions have been adopted [1]: the lithospheric plate and the underlying mantle are considered as the non-compressible Newtonian liquid with a very high viscosity. The temperature at a boundary between the mantle and the plate is constant and equals to the temperature of solid state </span><em><span>T</span></em><em><sub><span>s</span></sub></em><span>. The thermal conductivity </span><em><span>, </span></em><span>the viscosity of the substance and the heat flux </span><em><span>q</span></em><em><sub><span>v</span></sub></em><span> are determined with account of their temperature dependence: </span><br />
<span>1. </span><strong></strong><img src="http://content.snauka.ru/web/65807_files/073L0M4YO.gif" alt="" width="213" height="61" /><br />
<span>Index 1 denotes the lithosphere parameters, 2 &#8211; the mantle parameters. The dependence of the density p on the temperature of the medium is assumed to be</span></p>
<p><img src="http://content.snauka.ru/web/65807_files/01GA1IKHF.gif" alt="" width="160" height="58" /></p>
<p><span>2. Border between lithosphere and mantle is isotherm of solid phase with value of temperature Ts.</span><br />
<span>3. The relative quantity of the solid phase (characterizing melting and crystallization of the substance) contained in the mantle or lithosphere is determined depending on the state of the substance (a solid state with a temperature </span><em><span>T</span></em><em><sub><span>S</span></sub></em><span> or a liquid state with a temperature </span><em><span>T</span></em><em><sub><span>L</span></sub></em><span>). The relative quantity of the solid phase , depending of temperature, approximates by cubic spline [1]:</span></p>
<p><img src="http://content.snauka.ru/web/65807_files/0NZO12ZTU.gif" alt="" width="336" height="125" /><br />
<span>At &lt; 0.95 it is assumed that the substance is in the melted (liquid) state, while at &gt; 0.95 &#8211; in the solid state. A set of parameters for the lithosphere and the mantle used for the calculations are listed in the Table.</span><br />
<span>Following the hypothesis propounded in 1960 by H. Hess, the lithospheric plate motions are going on in a rectilinear manner starting from the areas of formation of the plates up to the zones of under thrusting, which allows us to solve the problem in a plane vertical layer. It results from systematic investigations of the island arc and continental margin zones that the depth of subsidence of the under thrusting plate does not exceed 700 km. Therefore, the extent of the area calculated along the Y-axis is assumed to be 1000 km. According to the results obtained, the extent of the calculated area along the X-axis is assumed to be 3000 km.</span></p>
<div align="center"><span>Table. </span><span>Thermophysical properties</span></div>
<div style="text-align: center;">
<table style="border-collapse: collapse;" border="0" align="center">
<colgroup>
<col style="width: 269px;" />
<col style="width: 6px;" />
<col style="width: 114px;" />
<col style="width: 76px;" />
<col style="width: 16px;" />
<col style="width: 164px;" />
<col style="width: 4px;" /></colgroup>
<tbody valign="top">
<tr>
<td style="padding-left: 7px; padding-right: 7px; border-top: solid 1.5pt; border-bottom: solid 1pt;" colspan="2"><span>Physical properties<br />
</span></td>
<td style="padding-left: 7px; padding-right: 7px; border-top: solid 1.5pt; border-bottom: solid 1pt;" colspan="2">
<p style="text-align: center;"><span>Lithosphere<br />
</span></p>
</td>
<td style="padding-left: 7px; padding-right: 7px; border-top: solid 1.5pt; border-bottom: solid 1pt;" colspan="3">
<p style="text-align: center;"><span> Mantle</span></p>
</td>
</tr>
<tr>
<td style="padding-left: 7px; padding-right: 7px;" colspan="2"><span>Viscosity </span><span>m</span><span> (Pa s) </span></td>
<td style="padding-left: 7px; padding-right: 7px;">
<p style="text-align: center;"><span> 10<sup>22</sup></span></p>
</td>
<td style="padding-left: 7px; padding-right: 7px;"></td>
<td style="padding-left: 7px; padding-right: 7px;"></td>
<td style="padding-left: 7px; padding-right: 7px;">
<p style="text-align: center;"><span> 10<sup>20</sup></span></p>
</td>
</tr>
<tr style="height: 123px;">
<td style="padding-left: 7px; padding-right: 7px; border-bottom: solid 1.5pt;"><span>Thermal conductivity </span><span>l</span><span> (Wt/mK)<br />
</span><span>Density </span><span>r</span><span> (kg/m<sup>3</sup>)<br />
</span><span>Heat flux q<sub>v</sub> (Wt/m<sup>3</sup>)<br />
</span></p>
<p><span>Specific heat capacity C<sub>p </sub>(J/kgK)<br />
</span></p>
<p><span>Volumetric expansion coefficient </span><span>b</span><span> (1/K)<br />
</span></p>
<p><span>Heat of melting L<sub>F</sub> (J/kg)</span></td>
<td style="padding-left: 7px; padding-right: 7px; border-bottom: solid 1.5pt;" colspan="2">
<p style="text-align: center;"><span> 3<br />
</span></p>
<p style="text-align: center;"><span> 3000<br />
</span></p>
<p style="text-align: center;"><span> 5</span><span>×</span><span>10<sup>-6<br />
</sup></span></p>
<p style="text-align: center;"><span> 1200<br />
</span></p>
<p style="text-align: center;"><span> 3</span><span>×</span><span>10<sup>-7</sup><br />
</span></p>
<p style="text-align: center;"><span> 4</span><span>×</span><span>10<sup>5</sup></span></p>
</td>
<td style="padding-left: 7px; padding-right: 7px; border-bottom: solid 1.5pt;"></td>
<td style="padding-left: 7px; padding-right: 7px; border-bottom: solid 1.5pt;"></td>
<td style="padding-left: 7px; padding-right: 7px; border-bottom: solid 1.5pt;">
<p style="text-align: center;"><span>5<br />
</span></p>
<p style="text-align: center;"><span> 3300<br />
</span></p>
<p style="text-align: center;"><span> 10<sup>-9<br />
</sup></span></p>
<p style="text-align: center;"><span> 1200<br />
</span></p>
<p style="text-align: center;"><span> 3</span><span>×</span><span>10<sup>-7</sup><br />
</span></p>
<p style="text-align: center;"><span> 4</span><span>×</span><span>10<sup>5</sup></span></p>
</td>
</tr>
</tbody>
</table>
</div>
<p><strong><span>3. Mathematical Model</span></strong></p>
<p><span>Fig. 1 shows physical setting of a problem [1]. The horizontal oceanic plate moves towards the continental plate with a constant velocity </span><em><span>U</span></em><em><sub><span>0</span></sub></em><span>, and subsides in the asthenosphere in the trench zone at an angle to the land surface with the same velocity. In turn, the continental plate moves towards the oceanic plate with a velocity </span><em><span>U</span></em><em><sub><span>k</span></sub></em><span>. Most often the lithospheric plates are subsiding in the subduction zones at an angle of 45°, though in some sectors of the island arcs the angles of subsidence from 30° to 90° have been marked. Here </span><em><span>U</span></em><em><sub><span>k</span></sub></em><span> - velocity of a continental plate, </span><em><span>U</span></em><em><sub><span>0</span></sub></em><span> - velocity of oceanic (lithospheric) plate; index 1 – lithosphere parameters, 2 – mantle parameters; &#8211; angle of immersing of oceanic plate; </span><em><span>Г1, Г2, Г3</span></em><span> - right, lower and left border of a trench, on which the plate is immersed, accordingly. </span></p>
<div align="center"><img src="http://content.snauka.ru/web/65807_files/90.gif" alt="" width="576" height="384" /><br />
<em><span>Fig. 1. Physical formulation of the problem</span></em></div>
<p><span>Location of trough, on which the plate is immersed, is considered equal </span><em><span>Lx /2</span></em><span>. The lower border </span><em><span>Г2</span></em><span>, up to which the velocity of immersing of a plate is known, is determined on the interval of temperature melting. At achievement of melting temperature (liquid) </span><em><span>T</span></em><em><sub><span>L</span></sub></em><span> the lithospheric plate melts and depth of its immersing in mantle is determined.</span><br />
<span>The mathematical statement of a task describing convection in subduction zone includes the equations of movement of an incompressible liquid in the Boussinesq approximation, continuity and energy with account internal heat sources. The governing dimensionless equations can be written as [1]:</span></p>
<div align="center"><img src="http://content.snauka.ru/web/65807_files/92.gif" alt="" width="366" height="48" /><span>,</span><br />
<img src="http://content.snauka.ru/web/65807_files/93.gif" alt="" width="144" height="50" /><span>,</span><br />
<img src="http://content.snauka.ru/web/65807_files/93(1).gif" alt="" width="265" height="45" /><span>.</span></div>
<p><span>Where</span><br />
<img src="http://content.snauka.ru/web/65807_files/93(2).gif" alt="" width="56" height="44" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(3).gif" alt="" width="52" height="44" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(4).gif" alt="" width="56" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(5).gif" alt="" width="53" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(6).gif" alt="" width="81" height="46" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(7).gif" alt="" width="56" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/93(8).gif" alt="" width="62" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94.gif" alt="" width="54" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(1).gif" alt="" width="106" height="48" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(2).gif" alt="" width="66" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(3).gif" alt="" width="73" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(4).gif" alt="" width="60" height="46" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(5).gif" alt="" width="69" height="44" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(6).gif" alt="" width="89" height="46" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(7).gif" alt="" width="86" height="45" /><span>. </span><img src="http://content.snauka.ru/web/65807_files/94(8).gif" alt="" width="116" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/94(9).gif" alt="" width="96" height="46" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/95.gif" alt="" width="172" height="48" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/95(1).gif" alt="" width="77" height="46" /><span> </span><span>Stefan, Reynolds, Grashof and Peclet numbers.</span><br />
<img src="http://content.snauka.ru/web/65807_files/95(2).gif" alt="" width="244" height="88" /><span> </span><img src="http://content.snauka.ru/web/65807_files/95(3).gif" alt="" width="228" height="88" /><span>.</span></p>
<p><img src="http://content.snauka.ru/web/65807_files/95(4).gif" alt="" width="278" height="122" /><span>.</span><br />
<img src="http://content.snauka.ru/web/65807_files/96.gif" alt="" width="368" height="50" /><span>, </span><span>H = [0;1]</span><span> </span><span>the dimensionless mantle depth.</span><span> </span></p>
<p><span>Boundary conditions: </span><br />
<img src="http://content.snauka.ru/web/65807_files/96(1).gif" alt="" width="17" height="18" /><em><span> = 0 </span></em><span>at</span><em><span> Y = 1; </span></em><img src="http://content.snauka.ru/web/65807_files/96(2).gif" alt="" width="17" height="18" /><em><span> = 1 </span></em><span>at</span><em><span> Y = 0; </span></em><img src="http://content.snauka.ru/web/65807_files/96(3).gif" alt="" width="54" height="41" /><em><span> </span></em><span>at</span><em><span> X = 0 </span></em><span>and</span><em><span> X = Lx/Ly.</span></em><br />
<img src="http://content.snauka.ru/web/65807_files/96(4).gif" alt="" width="108" height="46" /><span> </span><img src="http://content.snauka.ru/web/65807_files/96(5).gif" alt="" width="226" height="46" /><span>, </span><em><span>(k = 1,2,3)</span></em><span> at border Г1, Г2, Г3 (fig. 1).</span><br />
<img src="http://content.snauka.ru/web/65807_files/97.gif" alt="" width="54" height="22" /><span> at border Г1, Г3; </span><img src="http://content.snauka.ru/web/65807_files/97(1).gif" alt="" width="89" height="22" /><span> at border Г2.</span><br />
<img src="http://content.snauka.ru/web/65807_files/97(2).gif" alt="" width="73" height="46" /><span> at </span><em><span>X = [0; (Lx/2Ly - Lp/2Ly)]; Y = 1.</span></em><br />
<img src="http://content.snauka.ru/web/65807_files/97(3).gif" alt="" width="64" height="45" /><span> at </span><em><span>X = [(Lx/2Ly - Lp/2Ly); Lx/Ly]; Y = 1.</span></em><br />
<img src="http://content.snauka.ru/web/65807_files/97(4).gif" alt="" width="56" height="45" /><span>, </span><img src="http://content.snauka.ru/web/65807_files/97(5).gif" alt="" width="64" height="48" /><span> at </span><em><span>X = [0; Lx/Ly]; </span></em><img src="http://content.snauka.ru/web/65807_files/97(6).gif" alt="" width="78" height="48" /><span> at</span><img src="http://content.snauka.ru/web/65807_files/97(7).gif" alt="" width="40" height="17" /><span>; </span><img src="http://content.snauka.ru/web/65807_files/97(8).gif" alt="" width="44" height="18" /><span> at </span><em><span>Y = 0.</span></em><br />
<img src="http://content.snauka.ru/web/65807_files/97(9).gif" alt="" width="150" height="68" /><span> at </span><img src="http://content.snauka.ru/web/65807_files/98.gif" alt="" width="18" height="22" /><span> (fig. 1). </span><br />
<img src="http://content.snauka.ru/web/65807_files/98(1).gif" alt="" width="270" height="46" /><span> on </span><em><span>Г1, Г3</span></em><span> (fig. 1) and inside a trench.</span><br />
<span>For intensity of a vortex </span><em><span>W</span></em><span> the boundary conditions were calculated with the use of boundary conditions for stream function. In accounts the non-uniform grid with a condensation in trench region and at the upper boundary of the area (</span><em><span>Y </span></em><span>= 1) was applied.</span><br />
<span>Dimensionless local Nusselt numbers on top (Y=1) and bottom (Y=0) to border of calculated area were determined by the expression </span><img src="http://content.snauka.ru/web/65807_files/98(2).gif" alt="" width="137" height="41" /><span> (the derivative was calculated on three points with the second order of approximation).</span><br />
<span>The calculations were performed on a nonuniform grid with concentration nodes in the chute region, day surface and vertical boundaries of the computational domain (fig. 2).</span></p>
<div align="center"><img src="http://content.snauka.ru/web/65807_files/111.gif" alt="" width="413" height="216" /><br />
<em><span>Fig. 2. The computational grid</span></em></div>
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