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contributor authorFRITZ, S.
contributor authorMacDONALD, T. H.
date accessioned2017-06-09T15:57:04Z
date available2017-06-09T15:57:04Z
date copyright1962/06/01
date issued1962
identifier issn0027-0644
identifier otherams-57306.pdf
identifier urihttp://onlinelibrary.yabesh.ir/handle/yetl/4197628
description abstractNormal-incidence solar radiation values were measured during the IGY at the South Pole and Little America (Antarctica), at Mauna Loa (Hawaii), Tucson (Arizona), and Blue Hill Observatory (Massachusetts); some results are given in tables and graphs. Essential differences among them are discussed. The radiation data at Tucson and Blue Hill are appreciably lower than at the other stations. The radiation, corrected for solar distance, is similar at the Antarctic stations to the radiation measured at Mauna Loa. However, the actual measured values in summer are higher at the South Pole than at Mauna Loa, because the sun is closer to the earth in the Southern Hemisphere summer. The ?extrapolated turbidity factor? is over 2.5 at Tucson and Blue Hill, but averages 2.0 or less at the other stations with the lowest values of about 1.5 at the South Pole.
publisherAmerican Meteorological Society
titleSOME NORMAL-INCIDENCE SOLAR RADIATION OBSERVATIONS DURING THE IGY
typeJournal Paper
journal volume90
journal issue6
journal titleMonthly Weather Review
identifier doi10.1175/1520-0493(1962)090<0241:SNSROD>2.0.CO;2
journal fristpage241
journal lastpage244
treeMonthly Weather Review:;1962:;volume( 090 ):;issue: 006
contenttypeFulltext


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