Smithsonian miscellaneous collections . Z / N \ / \ — t 3 - 2 - 1 0 *l *2 *3 *4 i i f , Figs. 3 and 4.—Time relations between maxima and minima in the solar constantand solar faculae. Means of faculae and solar constants for the 5 days before and the 5days after the dates of 72 selected days of maxima and 82 days of minima of solarconstants. ks he V • flSfc 11/ ..-??13 50 75 Sunspot numbers ?12^—^ (The number near each pointindicates the number of monthlymeans included in each group.) 125 So 17T Fig. 5.—Monthly mean values of the solar constant compared with monthly means ofsunspot
Smithsonian miscellaneous collections . Z / N \ / \ — t 3 - 2 - 1 0 *l *2 *3 *4 i i f , Figs. 3 and 4.—Time relations between maxima and minima in the solar constantand solar faculae. Means of faculae and solar constants for the 5 days before and the 5days after the dates of 72 selected days of maxima and 82 days of minima of solarconstants. ks he V • flSfc 11/ ..-??13 50 75 Sunspot numbers ?12^—^ (The number near each pointindicates the number of monthlymeans included in each group.) 125 So 17T Fig. 5.—Monthly mean values of the solar constant compared with monthly means ofsunspot numbers for the same days. 5 - i . < j - t : i 1 / 0 r - > , i ( A ) A 3 /2 M « • • » ; i 1 A 9 l ! *« lE Av . Ay \ \ *\J 0 \ /~v \ <i \s * 1 j /\ t [7 ; * --^ \ S» s / k / < /a / I v. J L V/l 2 3 \ \ / % // \ \ \ A r\ t \ ? \ / n S , ! /1\ A . 1 S / ? \ /\ \\ i 2 A^- // \ \ y \ °i i \ 1 / i i 1 V \ \* \\ \ • \/ V «• / \ \ 1 V V X. 6 4 ! c - - f < . » i-> 5 l 0 I H y V \\ ,.-,, „ -^ v / \ \ 1 \- /.-J -\ \ / -> •.„ S- \ r-S v^« •y a 7 / 9 .---. / \ \ / \ / \ f k / \ — s —- 7 \ \ / ??? m 1 y ,/ \ s -^ s s^ A \ J x /? 1! n 5 4 . > 1 1 AS- A _ tN 7, ^X. »?» y *2 \ \ i 2 f r J 7 sy s -,i- \\ / \ 7 t: { 0 /A // J I Cj / \ \ / s • \ VI \ / 10 *~ i 12 7 •5 / _y \ • / ?^ s / /- *V .s , /, . -N \ / ^ V ^ / \ \ ,-- / ^ \ Y / S / */ \ / /< / * L \ -v / Nr r %=* \ j \ / S V V. ,-- Fig. 6.—Average marches of temperature departures, Fahr., at Washington, D. C,accompanying sequences of solar change (a) of the solar constant in years 1924 to1936; (b) of character figures for solar calcium flocculi in years 1910 to 1937, formonths January to December. Ordinates are temperature departures; abscissae a
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