Sains Malaysiana 47(11)(2018): 2877–2885

http://dx.doi.org/10.17576/jsm-2018-4711-31

 

Measuring the Sun Depression Angle of Dawn with a DSLR Camera

(Mengukur Sudut Junaman Matahari bagi Fajar menggunakan Kamera DSLR)

 

KASSIM BAHALI1*, ABDUL LATIF SAMIAN1, NAZRI MUSLIM2 & NURUL SHAZANA ABDUL HAMID3

 

1Institute of the Malay World & Civilization (ATMA), Universiti Kebangsaan Malaysia, 43600 UKM Bangi, Selangor Darul Ehsan, Malaysia

 

2Pusat Citra Universiti, Universiti Kebangsaan Malaysia, 43600 UKM Bangi, Selangor Darul Ehsan, Malaysia

 

3School of Applied Physics, Faculty Science and Technology, Universiti Kebangsaan Malaysia, 43600 UKM Bangi, Selangor Darul Ehsan, Malaysia

 

Diserahkan: 15 Mei 2018/Diterima: 27 Julai 2018

 

ABSTRACT

The first visibility of the dawn occurs at a definite angle of the sun depression, Do which is used to calculate the fajr (dawn) prayer time. Dawn observations were carried out using Digital Single-lens Reflex (DSLR) camera in the period from February to December 2017 at several locations in both Malaysia and Indonesia (Lat. between 2.0° - 7.0° N, Long. 95.0°-106.0°E). Within the observational period, 64 days of the dawn luminance at horizon were recorded with backgrounds of both sea and land. The purpose of these observations was to determine the sun depression angle Do at the first moment when the dawn is seen using a DSLR camera. The results indicated that Do can be determined using a DSLR camera. The value of Do is between -14.5° and -18.5° with a mean value of -16.67° and standard deviation of 0.9992. This suggests that the new sun depression angle Do for dawn prayer is -17.0°.

 

Keywords: Dawn; digital camera; sun depression angle

 

ABSTRAK

Fajar mula-mula kelihatan berlaku pada suatu sudut junaman matahari Do yang tertentu yang digunakan untuk menghitung waktu solat subuh. Pencerapan fajar telah dilakukan menggunakan kamera digital kanta pemantul tunggal (DSLR) dalam tempoh dari Februari hingga Disember 2017 di beberapa lokasi di Malaysia dan Indonesia (Lat. di antara 2.0° - 7.0° U, Long. 95.0°-106.0°T). Dalam tempoh tersebut, 64 data cerapan kecerahan fajar di ufuk laut dan daratan telah direkodkan. Tujuan pencerapan ini adalah untuk menentukan sudut junaman matahari Do ketika fajar mula-mula kelihatan dengan kamera DSLR. Keputusan kajian menunjukkan Do boleh ditentukan dengan kamera DSLR dan nilai Do di antara -14.5° hingga -18.5° dengan min -16.67° dan sisihan piawai 0.9992. Dengan hal demikian, dicadangkan nilai sudut junaman baharu Do bagi solat subuh ialah -17.0°.

 

Kata kunci: Fajar; kamera digital; sudut junaman matahari

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*Pengarang untuk surat-menyurat; email: kassimhb@gmail.com

 

 

 

 

 

 

 

 

 

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