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preface to fifteenth edition

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2.70 SECTION 2<br />

Example 3.<br />

25<br />

1.2500 :<br />

4<br />

To find the specific gravity at 20/4C of a liquid which has a specific gravity of<br />

Since the density of water at 4C, is equal<strong>to</strong> 1, specific gravity 25/4 d25<br />

1.2500; and,<br />

specific gravity 20/4 d<br />

20.<br />

Substitution in Equation 3, with d<br />

t<br />

1.2500; and, with F t<br />

at 25C, from the table, equal <strong>to</strong><br />

0.99705, gives<br />

Sp. gr. 25/25 S 1.2500 0.99705<br />

Substitution of this value for S in Equation 2, with F t<br />

at 20C, from the table, equal <strong>to</strong> 1.0036,<br />

gives<br />

20<br />

Sp. gr. 20/4 d (1.2500 0.99705) 1.0036 1.2582<br />

15<br />

Example 4. To find the density at 25C of a liquid which has a specific gravity of 1.250015:<br />

Since the density of water at 15C 0.99910,<br />

Substitution in Equation 3, with<br />

15<br />

d sp. gr. 15/15 0.99910 1.2500 0.99910<br />

F t<br />

at 15C, from the table, equal <strong>to</strong> 1.0102, gives<br />

Sp. gr. 25/25 S (1.2500 0.99910) 1.0102<br />

Substitution of this value for S in Equation 2, with F t<br />

at 25, from the table, equal <strong>to</strong> 0.99705,<br />

gives<br />

26 t<br />

d d (1.2500 0.99910 1.0102) 0.99705 1.2326<br />

2.1.3 Barometry and Barometric Corrections<br />

In principle, the mercurial barometer balances a column of pure mercury against the weight of the<br />

atmosphere. The height of the column above the level of the mercury in the reservoir can be measured<br />

and serves as a direct index of atmospheric pressure. The space above the mercury in a barometer<br />

tube should be a Torricellian vacuum, perfect except for the practically negligible vapor pressure of<br />

mercury. The perfection of the vacuum is indicated by the sharpness of the click noted when the<br />

barometer tube is inclined. A barometer should be in a vertical position, suspended rather than<br />

fastened <strong>to</strong> a wall, and in a good light but not exposed <strong>to</strong> direct sunlight or <strong>to</strong>o near a source of<br />

heat. The standard conditions for barometric measurements are 0C and gravity as at 45 latitude<br />

and sea level. There are numerous sources of error, but corrections for most of these are readily<br />

applied. Some of the corrections are very small, and their application may be questionable in view<br />

of the probably larger errors. The degree of consistency <strong>to</strong> be expected in careful measurements is<br />

about 0.13 mm with a 6.4-mm tube, increasing <strong>to</strong> 0.04 mm with a tube 12.7 mm in diameter.<br />

In reading a barometer of the Fortin type (the usuallabora<strong>to</strong>ry instrument for precision measurements),<br />

the procedure should be as follows: (1) Observe and record the temperature as indicated<br />

by the thermometer attached <strong>to</strong> the barometer. The temperature correction is very important and may<br />

be affected by heat from the observer’s body. (2) Set the mercury in the reservoir at zero level, so<br />

that the point of the pin above the mercury just <strong>to</strong>uches the surface, making a barely noticeable<br />

dimple therein. Tap the tube at the <strong>to</strong>p and verify the zero setting. (3) Bring the vernier down until<br />

the view at the light background is cut off at the highest point of the meniscus. Record the reading.<br />

The corrections <strong>to</strong> be made on the reading are as follows: (1) Temperature, <strong>to</strong> correct for the<br />

difference in thermal expansion of the mercury and the brass (or glass) <strong>to</strong> which the scale is attached.

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