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The manner of using it is explained in connection with the table. * It should be noted that CWis not equal to EV^ A^and F referring here to points on the developed parallels. t Compies Rendus, Paris, 1850, vol. xxv. p. 309. ^^ hkI OOoIp Digitized by^ >8' CIV EXPLANATION OF SOURCE AND USE OF TABLES. Table 31 gives the mean astronomical refraction in terms of the apparent alti- tude of a star or other object outside the earth's atmosphere. It is taken from Vega's 7-place table of logarithms. Its ...use will be evident from the following example : — Apparent altitude of star =r 34° 17' n."; Refraction = i' 24/'^ — » X i."i = i 24.1 True altitude of star =34 15 48.6 Tables 3a and 33 facilitate the interconversion of arc and time. They are taken from the *' Smithsonian Meteorological Tables" (the first volume of this series). The following examples illustrate their use : — (i.) To convert 68® 29' 48."8 into time we have from Table 32 — 68** = 4^ 32™ GO- 29' = I 56 48" = 3-20 o/'8 = .OS Equivalent in time = 4 33 59.25 (2.) To convert 5^ 43" 28.*8 into arc we have from Table 33 — 5 — 75 ^^^ 00 43" = 10 45 00 28' = 7 00 0/8 = 12 Equivalent in arc = 85 52 12 Tables 34 and 35 facilitate the interconversion of mean solar and sidereal time intervals.
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