تضمن البحث دراسة للتغيرات اليومية و الشهرية لشدة الإشعاع الشمسي الكلي في مدينة حمص عام 2013, و ذلك بالقياس المباشر لهذه الشدة، بينت الدراسة أن الشدة تتغير لتأخذ قيماً عظمى في الصيف و قيماً صغرى في الشتاء، و يعود الاختلاف في القيم المقاسة صيفاً عنها شتاءً لاعتمادها على تغير ميل الشمس و ضمناً زاوية السمت الشمسية, تكون هذه الزاوية أكبر ما يمكن شتاءً و المسار الضوئي أعظمي ، فتزداد عمليتا التبعثر و الامتصاص، أما صيفاً فتكون زاوية الميل أصغر ما يمكن و المسار الضوئي أصغري ، و امتصاص الإشعاع الشمسي و تبعثره يكون أصغرياً.
This research includes a detailed study of the daily and monthly
changes to the intensity of total solar radiation in the city of Homs
(34.75N °, 36.7 E °), and a direct measurement of the intensity. The
study shows that intensity increases to maximum values in summer
1100w / m2, and drops to lesser values in winter 600 w / m2. The
difference between the measured values in summer and winter is
due to: a change in the inclination of the sun, and implicitly solar
azimuth z. This angle is at its greatest in winter and the optical
path is at the maximum. Thus, the processes of scattering and
absorption increase. In summer, the inclination angle is at its lowest
and the optical path is at the minimum. Thus, the absorption and
scattering of solar radiation are at the minimum.
References used
Rodhn, H. A. (1990).,” A comparison of the contribution of various gases to the greenhouse effect“, Science, 248: 1217
Strahler, A.N. (1969): Physical geography, John– Wiley & Sons, New York, USA
Muneer T. , (2004), “Solar radiation and daylight models”, 2nd edition, Elsevier Ltd
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In th
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