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2.2. THEORY OF ERRORS<br />

2.2.1. Types of Errors<br />

If the measurements are physically derived using measuring<br />

tools, they are referred to as direct; if derived using a formula,<br />

they are indirect. For example, determining the length of an<br />

object with a metric ruler is a direct measurement, while determining<br />

the moment of inertia using the formula I = mr', is an indirect<br />

measurement.<br />

The measured value for a quantity always differs from the true<br />

value for the quantity. The reasons for the difference are instrumental<br />

measurement errors (due to the imperfection of the measuring<br />

instrument) and personal errors (due to measuring errors by<br />

the individual). Another method for classifying errors is based on<br />

their properties. An error is systematic if it is constant over several<br />

measurements or random if it changes during the measurements.<br />

The following definitions more precisely describe these<br />

terms.<br />

Error - the difference between the determined value of a physical<br />

quantity and the true value.<br />

The foregoing classification of measurement errors is based on<br />

the cause of the errors.<br />

Systematic errors are caused by the imperfection of measuring<br />

methods and inaccuracy of instruments. These errors remain constant<br />

or change in a regular fashion in repeated measurements of<br />

one and the same quantity.<br />

Random errors mean the individual errors that are given rise to<br />

the person performing the measurements; they include errors<br />

owing to incorrect reading of the tenth graduation of an instrument<br />

scale, small changes of the measurement conditions, asymmetric<br />

placement of the indicator mark etc. These errors are changing<br />

in an irregular fashion in repeated measurements of one and<br />

the same quantity.<br />

2.2.2. Errors in Direct Measurements<br />

Let x I' X 2'<br />

X 3'<br />

x n<br />

denote the raw data derived from experimental<br />

observations. The arithmetic mean «x» is the sum of observations<br />

divided by the number (n) of observations:<br />

n<br />

LXi<br />

Y. + Y- + Y- +...+ X . I<br />

< X > = 0'1 OV2 oVJ n =-'-=-- (2.1)<br />

n<br />

n<br />

The difference between a data point and the mean is referred to<br />

as a deviation (8):<br />

8. = x. - < x > (2.2)<br />

I<br />

I<br />

Dispersion or variance (0'2) is defined as the sum of the<br />

squared deviations divided by n - I:<br />

n<br />

2<br />

LD j<br />

a 2 = ..i..::L-­ (2.3)<br />

n-l<br />

Sample standard deviation (0') is defined as the square root of<br />

the dispersion by the following formula:<br />

0'=<br />

n<br />

LS;<br />

i;1 (2.4)<br />

n-l<br />

Confidence interval is the difference between the largest and<br />

smallest observations in a sample.<br />

Confidence interval of systematic error (6) is the smallest division<br />

of the measuring instrument.<br />

Confidence interval of random error (~) is defined by the following<br />

formula:<br />

o<br />

.!1 = t<br />

n<br />

:L S;<br />

i;1 (2.5)<br />

n(n-l)<br />

10<br />

11

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