A finite and exact expression for the refraction of an atmosphere nearly resembling that of the earth
Having shown that if the pressure of the .atmosphere he represented either by the square, or by the cube of the square root of the density, the astronomical refraction may be attained in a finite equation; and having adverted to Mr. Ivory’s computation of the refraction with the assistance of converging series, and several transformations from an equation which expresses the pressure in terms of the density and of its square, Dr. Young proceeds to observe, that if we substitute for the simple density the cube of its square root, we shall represent the constitution of the most important part of the atmosphere with equal accuracy, although this expression supposes the total height somewhat smaller than the truth; and that we shall thus obtain a direct equation for the refraction, which agrees very nearly with Mr. Ivory’s table, and still more accurately with that in the Nautical Almanac, and with the French tables. At the horizon the refraction is equal to 33' 49"· 5, which is only l''·5 less than the quantity assigned by the French tables and in the Nautical Almanac; while Mr. Ivory makes it 34' 17"·5. Again, for the altitude 5° 44' 21", we obtain 8' 49"'·5 for the refraction; while the Nautical Almanac gives us 8' 53", and Mr. Ivory’s table S' 49"·6. The author, however, observes that there is no reason for proceeding to compute a new table by this formula, since the method employed for that in the Nautical Almanac is in all common cases more compendious; and even if it were desired to represent Mr. Ivory’s table by the approximation there employed, we might obtain the same results, with an error scarcely exceeding a single second, from an equation of the same form.