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Instructor: Welcome back everybody.
Towards the end of the last lecture,
we mentioned standardizing,
but didn't explain what it is and why we use it.
Before we understand this concept
we need to explain what a transformation is.
So a transformation is a way in which we can alter
every element of a distribution to get a new distribution
with similar characteristics.
For normal distributions we can use addition,
subtraction, multiplication, and division,
without changing the type of the distribution.
For instance, if we add a constant
to every element of a normal distribution
the new distribution would still be normal.
Let's discuss the four algebraic options
and see how each one affects the graph.
If we had a constant like three to the entire distribution
then we simply need to move the graph three places
to the right.
Similarly, if we subtract a number from every element
we would simply move our current graph
to the left to get the new one.
If we multiply the function by a constant
it will shrink that many times,
and if we divide every element by a number,
the graph will expand.
However, if we multiply or divide by a number
between zero and one, the opposing effects will occur.
For example, dividing by a half is the same as multiplying
by two, so the graph will shrink
even though we are dividing.
All right.
Now that you know what a transformation is,
we can explain standardizing.
Standardizing is a special kind of transformation
in which we make the expected value equal to zero
and the variance equal to one.
The distribution we get after standardizing
any normal distribution is called
a standard normal distribution.
In addition to the 68, 95, 99.7 rule,
a table exists which summarizes the most commonly
used values for the CDF of a standard normal distribution.
This table is known as the standard normal distribution
table or the Z-score table.
Okay, so far we have learned what standardizing is
and why it's convenient.
What we haven't talked about is how to do it.
First, we wish to move the graph either to the left
or to the right until it's mean equals zero.
The way we would do that is by subtracting the mean Mu,
from every element.
After this, to make the standardization complete
we need to make sure the standard deviation is one.
To do so, we would have to divide every element
of the newly obtained distribution
by the value of the standard deviation, sigma.
If we denote the standard normal distribution with Z,
then for any normally distributed variable Y,
Z equals Y minus Mu over sigma.
This equation expresses the transformation we
use when standardizing.
Amazing.
Applying this single transformation
for any normal distribution would result in a standard
normal distribution, which is convenient.
Essentially, every element of the non-standardized
distribution is represented in the new distribution
by the number of standard deviations it is
away from the mean.
For instance, if a value Y is 2.3 standard deviations
away from the mean, it's equivalent value Z
would be equal to 2.3.
Standardizing is incredibly useful when
we have a normal distribution.
However, we cannot always anticipate
the data is spread out that way.
A crucial fact to remember about the normal distribution
is that it requires a lot of data.
If our sample is limited, we run the risk of outliers
drastically affecting our analysis.
In cases where we have less than 30 entries,
we usually avoid assuming a normal distribution.
However, there is a small sample size approximation
of a normal distribution called
the student's T distribution.
And we are going to focus on that in our next lecture.
Thanks for watching.
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