EXPLANATION OF TABLES XIV TO XXI 



In the following tables are included all the observations at Indio (Table 

 XIV), at Lone Pine (Table XV), at Lone Pine Canyon (Table XVI), at 

 Mount San Antonio (Table XVII), at Mount San Gorgonio (Table XVIII), 

 at Mount Whitney (Table XIX), and at Mount Wilson (Table XX). Upon the 

 values given in these tables, the studies of the total radiation are based. In the 

 tables are given: (i) the date, (2) the time, (3) the temperature (0, (4) the 

 pressure of aqueous vapor (H), (5) the radiation of a black body (St) at the 

 temperature (t) (Kurlbaum's constant), (6) the observed effective radiation 

 (Rt), (7) the difference between St and Rt, here defined as being the radiation 

 of the atmosphere, (8) this radiation reduced to a temperature of 20 C, in 

 accordance with the discussion presented in chapter V: B (E 20O ), and finally 

 Remarks in regard to the general meteorological conditions prevailing at the 

 time of observation. With each night of observation is given the initials of the 

 observers : A. K. Angstrom, E. H. Kennard, F. P. Brackett, R. D. Williams, 

 and W. Brewster. 



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