A Treatise On the Sun's Radiation And Other Solar Phenomena, in Continuation of the Meteorological Treatise On Atmospheric Circulation And Radiation, 1915
A Treatise On the Sun's Radiation And Other Solar Phenomena, in Continuation of the Meteorological Treatise On Atmospheric Circulation And Radiation, 1915
Frank H Frank Hagar Bigelow
The book A Treatise On the Sun's Radiation And Other Solar Phenomena, in Continuation of the Meteorological Treatise On Atmospheric Circulation And Radiation, 1915 was written by author Frank H Frank Hagar Bigelow Here you can read free online of A Treatise On the Sun's Radiation And Other Solar Phenomena, in Continuation of the Meteorological Treatise On Atmospheric Circulation And Radiation, 1915 book, rate and share your impressions in comments. If you don't know what to write, just answer the question: Why is A Treatise On the Sun's Radiation And Other Solar Phenomena, in Continuation of the Meteorological Treatise On Atmospheric Circulation And Radiation, 1915 a good or bad book?
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Vol. II, Annals Smithsonian Institution, or the Astrophysical Journal, October, 1911, the method of reducing the original arbitrary units to the probable calories being given in Bulletin No. 3, p. 83. The values at the several wave lengths have been made as homogeneous as practicable in Table 79 and the corresponding curves are plotted on Fig. 25, where their mutual relations can be examined. The sums of the several columns are taken, and as they are com- parable there should be a common factor... to reduce the areas which are equivalent to the curves to the corresponding calories. Such a factor has been foimd to be 20.90. The factor used in Bui. No. 4, page 84, is 20.72, where the same table in part may be found. The lower portion of Table 79 contains the reductions in calories at the distance of the earth. Under " reduced " values the sums of the columns divided by the factor 20.9 are given; under " thermodynamics " are found the corresponding values, as deduced from the several independent discussions by thermodynamics, from bolometer observations, and from pyrheliometer reductions.
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