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    SOME NORMAL-INCIDENCE SOLAR RADIATION OBSERVATIONS DURING THE IGY

    Source: Monthly Weather Review:;1962:;volume( 090 ):;issue: 006::page 241
    Author:
    FRITZ, S.
    ,
    MacDONALD, T. H.
    DOI: 10.1175/1520-0493(1962)090<0241:SNSROD>2.0.CO;2
    Publisher: American Meteorological Society
    Abstract: Normal-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.
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      SOME NORMAL-INCIDENCE SOLAR RADIATION OBSERVATIONS DURING THE IGY

    URI
    http://yetl.yabesh.ir/yetl1/handle/yetl/4197628
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    • Monthly Weather Review

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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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