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A numerical research on the primary scattering of the sun's ray in the high atmosphere-2-


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Title: A numerical research on the primary scattering of the sun's ray in the high atmosphere-2-
Authors: Sato, Takao
Issue Date: 28-Feb-1969
Publisher: 長崎大学教育学部
Citation: 長崎大学教育学部自然科学研究報告. vol.20, p.67-85; 1969
Abstract: The author has investigated the primary scattering at 75 levels from 1 km to 38km height, the interval between neighboring two levels being 500m. Moreover the total solar energy is divided into twelve wavelength ranges, each of which has the partial energy equal to one twelfth of the total. Let To be each level point above explained and draw a line passing through To and making an angle θ1 with a line passing To and the earth's centre O. For convenience sake the line thus defined will be hereafter called θ1 line. Let T4 be the intersecting point of θ1 line with the earth's surface or its atmospheric upper limit, and T1, T2, T3 be three points which divide the line section between T0 and T4 into four equal lengths. Hereafter the above five points will be called in general Tπ. The author has researched and compared the primary scattering intensity which originates at Tn and reaches the level point To for 30°, 60° and 90° of the Sun's altitude h, determined each of two positions of the level point which take respectively max. and minimum value for each combination of the wavelength domains, θ1, h, and Tn.
URI: http://hdl.handle.net/10069/33092
ISSN: 0386443X
Type: Departmental Bulletin Paper
Text Version: publisher
Appears in Collections:No. 20

Citable URI : http://hdl.handle.net/10069/33092

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