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首页> 外文期刊>Journal of Molecular Liquids >Nanofluid thermal performance inside an absorber tube of LFR unit equipped with helical T-shape tape
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Nanofluid thermal performance inside an absorber tube of LFR unit equipped with helical T-shape tape

机译:LFR单元吸收管内的纳米流体热性能,配备螺旋T形胶带

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Entropy generation and thermal treatment of nanofluid through a solar unit with turbulent regime was examined in current investigation. To create the solar system, mirrors, trapezoidal cavity and tube have been utilized. The mirrors were situated above the ground with certain angles and tube was equipped with turbulator. Working fluid is homogeneous mixture of H2O-Al2O3 and temperature dependent variables were incorporated. Verification based on empirical correlation depicts the high accuracy of FVM simulation. Irreversibility components and friction resistance as well as Nu and thermal efficiency have been reported in outputs. The active variables are Twist ratio (TR), V-center dot. Width ratio (WR), T-in. Each factor which can augment the secondary flow makes the stronger impingement of fluid with wall and lower T-w appears. Such disruption of boundary layer causes cooling rate to augment. As V-center dot, TR and WR augment, wall temperature reduces about 1.01%, 0.063% and 0.0217%. With rise of TR and WR, pressure drop augments about 25.87% and 10.85%, respectively. Revolution number has greater impact on resistance of fluid than width of the tape. Augment of WR and TR makes friction resistance to augment about 7.46% and 29.68%. Considering greater WR and TR can able to more disturb the boundary layer and Nu can be augmented about 1.5% and 454%, respectively. Augmenting TR, WR and Re can reduce the irreversibility which is a pleasant result to obtain more available work. Augment of TR makes S-ge(n.h) to decline by 329% while S-gen.f rises about 1524%. Thermal performance decreases about 23.68% with rise of T-in while it augments about 0.027% and 0.11% with growth of WR and TR. respectively. (C) 2020 Elsevier B.V. All rights reserved.
机译:在当前的研究中,研究了纳米流体通过湍流区太阳能单元的熵产生和热处理。为了创造太阳系,人们使用了镜子、梯形腔和管。镜子位于地面上方,有一定角度,管子上装有涡流器。工作流体为H2O-Al2O3的均匀混合物,并考虑了温度相关变量。基于经验相关性的验证说明了FVM模拟的高精度。输出中报告了不可逆成分、摩擦阻力以及Nu和热效率。活动变量为扭转比(TR)、V中心点。宽度比(WR),T-in。每一个增大二次流的因素都会使壁面流体的冲击力更强,出现较低的T-w。这种边界层的破坏导致冷却速度增加。随着V中心点、TR和WR的增大,壁温分别降低约1.01%、0.063%和0.0217%。随着TR和WR的增加,压降分别增加约25.87%和10.85%。转数对流体阻力的影响大于胶带宽度。WR和TR的增大使摩擦阻力增大约7.46%和29.68%。考虑到更大的WR和TR可以对边界层产生更大的干扰,Nu可以分别增加约1.5%和454%。增大TR、WR和Re可以降低不可逆性,这是获得更多可用功的一个令人愉快的结果。TR的增加使S-ge(n.h)下降329%,而S-gen.f上升约1524%。热性能随T-in的增加而降低约23.68%,随WR和TR的增加而分别提高约0.027%和0.11%。(C) 2020爱思唯尔B.V.版权所有。

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