Modul photovoltaic cell merupakan perangkat elektronik yang merubah energi matahari menjadi energi listrik. Photovoltaic cell memiliki potensi membentuk sistem yang bersih, handal dalam sistem kelistrikan yang terukur dan terjangkau untuk masa depan. Penelitian ini membahas tentang pengujian performa keluaran listrik tegangan, arus, daya pada modul photovoltaic cell terhadap pengaruh intensitas cahaya. Penelitian dilakukan pada hari Jum’at 01 Juli 2022 di kecamatan Magetan. Penelitian dilakukan dengan menempatkan 2 modul photovoltaic cell yang disusun secara seri dengan penempatan sudut kemiringan 121°. Pada penelitian pengukuran dilakukan pada suhu udara lingkungan, intensitas cahaya, keluaran listrik photovoltaic cell yang berupa tegangan, arus, dan daya. Hasil penelitian menunjukkan intensitas cahaya mempengaruhi keluaran listrik dari photovoltaic cell. Nilai tegangan, arus, daya paling tinggi ditunjukkan pada pukul 12.18 WIB yaitu dengan tegangan 5.77 V, arus 0.27 A, dan daya 1.5579 W pada intensitas cahaya matahari sebesar 545.58 LUX.
This study aims to evaluate the performance of the trailing-edge (TE) cooling system in a gas turbine blade. Eddy Simulation (DES), based on the turbulence model of Spallart-Almaras (SA), was used to simulate the TE cooling system. A TE configuration with a five-row staggered pin-fin arrangement was employed as a computational domain. Three parameters, i.e., the coefficient of heat transfer on the pin-fins surface (hpin), the coefficient of discharge (CD), and the effectiveness of adiabatic film cooling were used to assess the performances. The findings denoted that the heat transfer fluctuations occurred on the surface of the pin-fins in each row. The discharge coefficient increased with the rising of the blowing ratio. The trend predicted data of effectiveness were in good agreement with realistic discrepancies compared to other researches, mainly for higher blowing ratio. The average effectiveness along the cut-off region was to be sensitive to the changes of the blowing ratio, which was attributed to the structures of turbulent flow along the mixing region.
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