PARAMETRIC STUDY OF TRANSIENT VERTICAL SOLAR CHIMNEY RESPONSES AS A PASSIVE VENTILATION SYSTEM
The solar chimney design is one of the many passive ventilation systems which received increasing attention from previous years prior. Though, transient solar chimney performance evaluations has yet to be conducted as much before due completion of this study. This report is then aimed at communic...
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Format: | Final Project |
Language: | Indonesia |
Online Access: | https://digilib.itb.ac.id/gdl/view/79540 |
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Institution: | Institut Teknologi Bandung |
Language: | Indonesia |
Summary: | The solar chimney design is one of the many passive ventilation systems which received
increasing attention from previous years prior. Though, transient solar chimney performance
evaluations has yet to be conducted as much before due completion of this study. This report
is then aimed at communicating results from a parametric study of transient vertical solar
chimney response as a passive ventilation system to propose extra design considerations and
or support findings within the literature.
This study leverages the respons surface methodology to fulfill its purposes. Data used
in the analysis are numerical results gained from fluid simulations for a period of one hour
under 500 Wm?2 of solar irradiation. Number of configurations evaluated is generated with
the Central Composite Design (CCD) of experiments for a total of nine cases. Considered
design parameters include chimney gap height and width, respectively modelled for values
ranging in 0.15–1 m and 1–2.5 m. Response surface models are fitted with regression for the
air velocity change per characteristic velocity of bouyant flow ratio and thermal efficiency.
Implications to other solar chimney performance metrics are then extrapolated from resulting
models.
Out of the two design parameters studied, namely chimney gap height and width, gap
height is found to have the most impact in the positive direction for air velocity and the
inverse for air temperature and the velocity growth to natural flow characteristic velocity ratio.
Channel gap height’s contribution in the model’s prediction accuracy of each responses are
reported to be 0.01 R2 (1%), 0.07 R2 (7.3%), and 0.37 R2 (70%) respectively. Interaction effect
contributions in the form of channel area and gap height to width ratio are found dominant in
the betterment of thermal efficiency prediction accuracy valuing at 0.35 R2 (71.4%). The main
inference of this study’s evaluation into solar chimney design parameter effects follows that
tightening chimney gap height would result in an overwhelmingly restrictive flow resistance,
baring any chance for occuring Bouyancy to develop the flow.
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