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ارزیابی پارامتر تابش خورشیدی ورودی به زمین حاصل از مدلهای تجربی و ماهوارهای | ||
تحقیقات آب و خاک ایران | ||
مقاله 151، دوره 50، شماره 2، خرداد و تیر 1398، صفحه 353-362 اصل مقاله (1.51 M) | ||
نوع مقاله: مقاله پژوهشی | ||
شناسه دیجیتال (DOI): 10.22059/ijswr.2018.250899.667839 | ||
نویسندگان | ||
حمیده نوری* 1؛ علی مختاری2؛ مجید وظیفه دوست3 | ||
1استادیار دانشکده مهندسی و فناوری کشاورزی، پردیس کشاورزی و منابع طبیعی دانشگاه تهران | ||
2دانشجو - دانشکده کشاورزی و منابع طبیعی دانشگاه تهران | ||
3گروه مهندسی آب دانشگاه گیلان، رشت، گیلان | ||
چکیده | ||
یکی از مهمترین فرآیندهای انتقال آب و انرژی در چرخه هیدرولوژیکی، تبخیر-تعرق است و تابش خورشیدی انرژی لازم برای انجام این فرآیند را تأمین میکند. درنتیجه تخمین هرچه دقیقتر میزان تبخیر-تعرق به تخمین دقیق میزان تابش خورشیدی وابسته است. این تحقیق با هدف ارزیابی میزان تابش خورشیدی در سطح زمین حاصل از سه روش معادلات تجربی (مدلهای آنگستروم و هارگریوز-سامانی) مدلهای فیزیکی دادهگواری شده (GLDAS/Noah، NCEP/NCAR)و مشاهدات ماهوارهای (CM-SAF)با استفاده از اندازهگیریهای زمینی صورت گرفته است. نتایج این تحقیق نشان داد مدل کالیبره شده آنگستروم با ضریب تبیین برابر با 9/0 و SEEبرابر با 58/2 بهترین عملکرد را داشته است. اما دقت این مدل وابسته به روش کالیبراسیون و وجود دادههای ساعات آفتابی است. محصول تابش سطح زمین مستخرج از GLDAS/Noah با ضریب تبیین و SEEبه ترتیب برابر با 87/0 و 5/3 بهترین کارایی را بعد از مدل واسنجی شده آنگستروم داشت. مدل GLDAS/Noahبا وجود برآورد 2/10 درصدی تابش خورشیدی بیش از اندازهگیری زمینی، در مناطقی که کمبود داده هواشناسی وجود دارد میتواند کارایی بسیار خوبی داشته باشد. | ||
کلیدواژهها | ||
آنگستروم؛ هارگریوز-سامانی؛ CM-SAF؛ GLDAS/Noah؛ NCEP/NCAR | ||
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