. The Ultra-Violet Band of Ammonia, and Its Occurrence in the Solar Spectrum . uously as the central maximum is approached,but in e and f it passes through a maximum as in a, * ( Astrophys. vol. 46, p. 85 (September, 1917), BAND OF AMMONIA, AND ITS OCCURRENCE IN THE SOLAR SPECTRUM. 359 Biege has found a hyperbolic relation between dx and m in the case of cyanogen,but it does not seem that this is applicable to the series under consideration, with thepossible exception of e and £ While it is possible to give approximate formulae of theusual type for these series over a large part of thei
. The Ultra-Violet Band of Ammonia, and Its Occurrence in the Solar Spectrum . uously as the central maximum is approached,but in e and f it passes through a maximum as in a, * ( Astrophys. vol. 46, p. 85 (September, 1917), BAND OF AMMONIA, AND ITS OCCURRENCE IN THE SOLAR SPECTRUM. 359 Biege has found a hyperbolic relation between dx and m in the case of cyanogen,but it does not seem that this is applicable to the series under consideration, with thepossible exception of e and £ While it is possible to give approximate formulae of theusual type for these series over a large part of their ranges, there seems little hope atpresent of finding any accurate formula which can be adapted to all of them. Onecan hardly resist the conclusion that there is some connection between the groups ofthree and the central maxima, but no numerical relation has yet been established. rrt 5 10 15 20 20 15 10 4 .^^—r™1™„T_-T«n—.—r_r__T__T_~j—j—^—j-^—j—,—p. i—i—-j—r™i—r—i—[—-t—r-t—r—\—r~T~i—i—j—r—i j r ;S 35 30 20. 7\philtrans02221688
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