# The Standard Normal Distribution

Site: | Saylor Academy |

Course: | MA121: Introduction to Statistics |

Book: | The Standard Normal Distribution |

Printed by: | Guest user |

Date: | Thursday, August 11, 2022, 12:38 AM |

## Description

This section talks about the standard normal curve and how to compute certain areas underneath the curve. This section also contains numerous exercises and examples.

##### LEARNING OBJECTIVES

- To learn what a standard normal random variable is.
- To learn how to use Figure 12.2 "Cumulative Normal Probability" to compute probabilities related to a standard normal random variable.

##### Definition

A **standard normal random variable** is a normally distributed random variable with mean and standard deviation . It will always be denoted by the letter .

The density function for a standard normal random variable is shown in Figure 5.9 "Density Curve for a Standard Normal Random Variable".

*Figure 5.9 Density Curve for a Standard Normal Random Variable*

To compute probabilities for we will not work with its density function directly but instead read probabilities out of Figure 12.2 "Cumulative Normal Probability" in Chapter 12 "Appendix". The tables are tables of cumulative probabilities; their entries are probabilities of the form . The use of the tables will be explained by the following series of examples.

##### EXAMPLE 4

Find the probabilities indicated, where as always denotes a standard normal random variable.

##### Solution:

a. Figure 5.10 "Computing Probabilities Using the Cumulative Table" shows how this probability is read directly from the table without any computation required. The digits in the ones and tenths places of , namely , are used to select the appropriate row of the table; the hundredths part of , namely , is used to select the appropriate column of the table. The four decimal place number in the interior of the table that lies in the intersection of the row and column selected, , is the probability sought: .

*Figure 5.10*

Computing Probabilities Using the Cumulative Table

a. The minus sign in makes no difference in the procedure; the table is used in exactly the same way as in part (a): the probability sought is the number that is in the intersection of the row with heading and the column with heading , the number . Thus

##### EXAMPLE 5

Find the probabilities indicated.

##### Solution:

a. Because the events and are complements, the Probability Rule for Complements implies that

Since inclusion of the endpoint makes no difference for the continuous random variable , , which we know how to find from the table. The number in the row with heading and in the column with heading is . Thus

Figure 5.11 "Computing a Probability for a Right Half-Line" illustrates the ideas geometrically. Since the total area under the curve is 1 and the area of the region to the left of is (from the table) , the area of the region to the right of must be .

*Figure 5.11*

Computing a Probability for a Right Half-Line

a. The minus sign in makes no difference in the procedure; the table is used in exactly the same way as in part (a). The number in the intersection of the row with heading and the column with heading is . This means that , hence

##### EXAMPLE 6

Find the probabilities indicated.

##### Solution:

a. Figure 5.12 "Computing a Probability for an Interval of Finite Length" illustrates the ideas involved for intervals of this type. First look up the areas in the table that correspond to the numbers (which we think of as to use the table) and . We obtain and , respectively. From the figure it is apparent that we must take the difference of these two numbers to obtain the probability desired. In symbols,

*Figure 5.12*

Computing a Probability for an Interval of Finite Length

a. The procedure for finding the probability that takes a value in a finite interval whose endpoints have opposite signs is exactly the same procedure used in part (a), and is illustrated in Figure 5.13 "Computing a Probability for an Interval of Finite Length". In symbols the computation is

*Figure 5.13*

Computing a Probability for an Interval of Finite Length

The next example shows what to do if the value of * that we want to look up in the table is not present there.*

##### EXAMPLE 7

Find the probabilities indicated.

##### Solution:

a. We attempt to compute the probability exactly as in Note 5.20 "Example 6 " by looking up the numbers and in the table. We obtain the value for the area of the region under the density curve to left of without any problem, but when we go to look up the number in the table, it is not there. We can see from the last row of numbers in the table that the area to the left of must be so close to 1 that to four decimal places it rounds to . Therefore

b. Similarly, here we can read directly from the table that the area under the density curve and to the left of is , but is too far to the left on the number line to be in the table. We can see from the first line of the table that the area to the left of must be so close to 0 that to four decimal places it rounds to . Therefore

The final example of this section explains the origin of the proportions given in the Empirical Rule.

##### EXAMPLE 8

Find the probabilities indicated.

##### Solution:

a. Using the table as was done in Note 5.20 "Example 6" (b) we obtain

Since has mean 0 and standard deviation 1 , for to take a value between and 1 means that takes a value that is within one standard deviation of the mean. Our computation shows that the probability that this happens is about , the proportion, given by the Empirical Rule for histograms that are mound shaped and symmetrical, like the bell curve.

b. Using the table in the same way,

This corresponds to the proportion for data within two standard deviations of the mean.

c. Similarly,

which corresponds to the proportion for data within three standard deviations of the mean.

This text was adapted by Saylor Academy under a Creative Commons Attribution-NonCommercial-ShareAlike 3.0 License without attribution as requested by the work's original creator or licensor.

1. Use Figure 12.2 "Cumulative Normal Probability" to find the probability indicated.

3. Use Figure 12.2 "Cumulative Normal Probability" to find the probability indicated.

5. Use Figure 12.2 "Cumulative Normal Probability" to find the probability indicated.

7. Use Figure 12.2 "Cumulative Normal Probability" to find the first probability listed. Find the second probability without referring to the table, but using the symmetry of the standard normal density curve instead. Sketch the density curve with relevant regions shaded to illustrate the computation.

9. The probability that a standard normal random variable takes a value in the union of intervals , which arises in applications, will be denoted or Use Figure 12.2 "Cumulative Normal Probability" to find the following probabilities of this type. Sketch the density curve with relevant regions shaded to illustrate the computation. Because of the symmetry of the standard normal density curve you need to use Figure 12.2 "Cumulative Normal Probability" only one time for each part.

1.

a. 0.0427

b. 0.9798

c. 0.5

d. 0.9826

e. 0.0516

f. 0.0091

3.

a. 0.1221

b. 0.5326

c. 0.2309

5.

a. 0.0823

b. 0.9147

c. 0.0000

d. 1.0000

7.

a. 0.1401, 0.1401

b. 0.3594, 0.3594

c. 0.8944, 0.8944

d. 0.9788, 0.9788

9.

a. 0.1970

b. 0.01980

c. 0.0500

d. 0.0020