Parametric analysis of a solar still with inverted V-shaped glass condenser
A parametric analysis of a solar still with an inverted V-shaped glass condenser is presented. Results are based on a new mathematical model obtained from a lumped-parameter analysis of the still, with an approach that makes each glass plate of the condensing system sensitive to orientation...
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VINCA Institute of Nuclear Sciences
2015-01-01
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doaj-3d95411e29e848528149a009a818a17b2021-01-02T00:44:53ZengVINCA Institute of Nuclear SciencesThermal Science0354-98362334-71632015-01-0119suppl. 257158010.2298/TSCI121029067R0354-98361400067RParametric analysis of a solar still with inverted V-shaped glass condenserRubio Eduardo0Fernández José L.1aUniversidad Autónoma de Aguascalientes, Centro de Ciencias de la Ingeniería, Cd. Universitaria Aguascalientes, Ags. C.P., MéxicoUniversidad Nacional Autónoma de México, Instituto de Ingeniería Cd. Universitaria, México D.F., MéxicoA parametric analysis of a solar still with an inverted V-shaped glass condenser is presented. Results are based on a new mathematical model obtained from a lumped-parameter analysis of the still, with an approach that makes each glass plate of the condensing system sensitive to orientation and depicts its thermal differences. Numerical computations are made to evaluate productivity and temperature differences between the condensing plates as a function of condenser orientation, extinction coefficient and thickness. From this study it was found a significant influence of incident solar radiation on the thermal performance of each condensing plate. Large extinction coefficients and thick glass plates increase absorption losses that result in an appreciable temperature difference. An extinction coefficient of 40 m-1 produces a temperature difference of 2.5°C between both condensers. A glass thickness of 10 mm may increase this temperature difference up to 3.5°C. With respect to the production, due to the still orientation, a difference of 8.7% was found for the condensing plates facing an east-west direction. The proposed model is able to reproduce the temperature and distillate production differences that arise between both condensers in good agreement with experimental data. The overall performance of the still, studied with this new approach, was also in accordance with the widely used traditional models for solar distillation. In addition, the condensing plates parameters of the still can be used to force a differential heating such that for the whole day the temperature of one condensing plate is always higher.http://www.doiserbia.nb.rs/img/doi/0354-9836/2015/0354-98361400067R.pdfsolar distillationmodelingcondensers differencessensitivity to orientation |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Rubio Eduardo Fernández José L. |
spellingShingle |
Rubio Eduardo Fernández José L. Parametric analysis of a solar still with inverted V-shaped glass condenser Thermal Science solar distillation modeling condensers differences sensitivity to orientation |
author_facet |
Rubio Eduardo Fernández José L. |
author_sort |
Rubio Eduardo |
title |
Parametric analysis of a solar still with inverted V-shaped glass condenser |
title_short |
Parametric analysis of a solar still with inverted V-shaped glass condenser |
title_full |
Parametric analysis of a solar still with inverted V-shaped glass condenser |
title_fullStr |
Parametric analysis of a solar still with inverted V-shaped glass condenser |
title_full_unstemmed |
Parametric analysis of a solar still with inverted V-shaped glass condenser |
title_sort |
parametric analysis of a solar still with inverted v-shaped glass condenser |
publisher |
VINCA Institute of Nuclear Sciences |
series |
Thermal Science |
issn |
0354-9836 2334-7163 |
publishDate |
2015-01-01 |
description |
A parametric analysis of a solar still with an inverted V-shaped glass
condenser is presented. Results are based on a new mathematical model
obtained from a lumped-parameter analysis of the still, with an approach that
makes each glass plate of the condensing system sensitive to orientation and
depicts its thermal differences. Numerical computations are made to evaluate
productivity and temperature differences between the condensing plates as a
function of condenser orientation, extinction coefficient and thickness. From
this study it was found a significant influence of incident solar radiation
on the thermal performance of each condensing plate. Large extinction
coefficients and thick glass plates increase absorption losses that result in
an appreciable temperature difference. An extinction coefficient of 40 m-1
produces a temperature difference of 2.5°C between both condensers. A glass
thickness of 10 mm may increase this temperature difference up to 3.5°C. With
respect to the production, due to the still orientation, a difference of 8.7%
was found for the condensing plates facing an east-west direction. The
proposed model is able to reproduce the temperature and distillate production
differences that arise between both condensers in good agreement with
experimental data. The overall performance of the still, studied with this
new approach, was also in accordance with the widely used traditional models
for solar distillation. In addition, the condensing plates parameters of the
still can be used to force a differential heating such that for the whole day
the temperature of one condensing plate is always higher. |
topic |
solar distillation modeling condensers differences sensitivity to orientation |
url |
http://www.doiserbia.nb.rs/img/doi/0354-9836/2015/0354-98361400067R.pdf |
work_keys_str_mv |
AT rubioeduardo parametricanalysisofasolarstillwithinvertedvshapedglasscondenser AT fernandezjosel parametricanalysisofasolarstillwithinvertedvshapedglasscondenser |
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