The aim of this paper is to show how the φ-f chart method can be implemented in Scilab. This model can be used to calculate the solar fraction for hot water production with respect to the global request.
The φ-f chart method is a simulation technique used in solar energy systems for heating and cooling. This method is particularly useful for sizing system components. The difficulty of sizing system’s components lies in the fact that these systems are influenced both by predictable data (e.g. collectors, storage tanks, ...) and unpredictable data such as weather data.
This Scilab code can be used to estimate the thermal performance of solar energy systems for domestic water, industrial process heating, and space heating systems where the thermodynamics cycle efficiency is independent of the heat supply temperature.
The complete Scilab code for simulating the described solar energy system is available to registered users only. For downloading the code visit: Registered Users Area .
| Attachment | Size |
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| Active Solar Energy Systems in Scilab | 674.55 KB |
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View the full image[画像:Schematic diagram of a closed loop solar energy system]
Schematic diagram of a closed loop solar energy system
Schematic diagram of a closed loop solar energy system
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View the full image[画像:Solar fraction with different collecting areas]
Solar fraction with different collecting areas
Solar fraction with different collecting areas
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View the full image[画像:Solar fraction with different specific storages]
Solar fraction with different specific storages
Solar fraction with different specific storages
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View the full image[画像:Solar fraction with different minimum temperature requirements]
Solar fraction with different minimum temperature requirements
Solar fraction with different minimum temperature requirements
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View the full image[画像:Solar fraction with three different tilt angles of solar collector]
Solar fraction with three different tilt angles of solar collector
Solar fraction with three different tilt angles of solar collector